This galaxy presents as a relatively smooth, elongated structure. The central region exhibits a significantly higher luminosity and a slightly redder hue, suggesting an older stellar population concentrated towards the core. Moving outwards from the core, the galaxy fades in intensity and displays a bluer tinge. The disk structure is apparent, extending along the major axis, although it is relatively featureless. There are no obvious signs of spiral arms, or significant dust lanes within this structure. The overall morphology is largely undisturbed, indicating a quiescent state without major mergers or interactions. The pronounced elongation of the galaxy indicates an elliptical shape, with a high probability of it being cigar shaped. There are no obvious signs of recent or ongoing major star formation outside of the central bulge, but there is a possibility of low-level star formation occurring throughout the galaxy.
