This galaxy exhibits a morphology consistent with an early-type spiral or lenticular galaxy viewed at a slight inclination. The central bulge is prominent and displays a smooth, yellowish-orange hue, indicative of an older stellar population and a lower rate of on-going star formation. Fainter, diffuse regions extend outwards from the central bulge, suggesting the presence of a disk component. There is minimal evidence of tightly wound spiral arms; instead, the disk appears relatively featureless and smooth. There may be a suggestion of a weak bar structure, though this is not definitive from the presented imagery. The overall shape is generally elliptical and shows a moderate degree of roundness. There do not appear to be any indications of tidal disturbances or recent merger activity, aside from a possible nearby interacting galaxy in the top right. The color distribution suggests a radial gradient, with bluer colors concentrated in the outer disk region, consistent with the presence of younger stars or residual star formation activity. The size of the galaxy appears moderate, fitting within the range of dwarf to intermediate-mass galaxies.
