The galaxy presents a somewhat elliptical morphology, though it exhibits noticeable disturbances in its structure. The central bulge is prominent and displays a yellowish hue, suggesting a population of older stars. There is a faint, diffuse disk component visible, appearing elongated. One side of the disk shows a slightly irregular extension, potentially indicating a minor interaction or tidal disturbance. Patches of bluer color are present, hinting at ongoing, though subdued, star formation activity within certain regions. Evidence suggests the galaxy could be in the process of merging or experiencing a close encounter, given the disrupted morphology and irregular features. The size appears moderate relative to other galaxies in the dataset, and it is neither particularly compact nor highly extended.
