The galaxy presents an elliptical morphology, though with a slight elongation suggestive of a possible disk component viewed at a shallow inclination. The central bulge is prominent, exhibiting a yellowish-orange hue, indicating an older stellar population. Moving outwards from the bulge, the galaxy transitions to a bluish color profile, hinting at more recent star formation occurring in the outer regions. There is a subtle hint of asymmetry or possible tidal features, but the resolution limits a definitive conclusion about interaction or merging events. The galaxy appears relatively smooth overall, with no obvious spiral arm structures visible, and no clear indication of intense ongoing star formation.
