The galaxy presents a somewhat elliptical morphology, exhibiting a smooth overall appearance with a dominant central bulge. The bulge displays a yellowish hue, suggesting a population of older, evolved stars. A fainter, bluer disk surrounds the bulge, indicating the presence of younger stars and some ongoing star formation. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, although there is a slight asymmetry to the outer regions of the disk, hinting at a possible minor interaction or internal irregularity. The color gradients suggest a radial distribution of stellar populations, with the bulge being more metal-rich and the disk containing a younger, bluer stellar population.
