The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth morphology without discernible spiral arm structures. The core region displays a bright, concentrated luminosity, indicative of a high stellar density. The galaxy appears to be relatively isolated, without signs of major mergers or tidal disturbances, though a slight asymmetry in the outer halo could hint at a past minor interaction. The color profile indicates a mix of stellar populations, with a central bulge that is likely dominated by older, redder stars, while the outer regions show bluer hues that suggest more recent, but perhaps suppressed, star formation activity. The overall structure suggests an evolved system approaching quiescence.
