The galaxy appears to be a relatively smooth, elliptical type. Its color is predominantly yellowish-orange, suggesting an older stellar population. The central bulge region exhibits a higher surface brightness and is more intensely yellow compared to the outer regions. There is little indication of spiral arm structure or significant dust lanes. The morphology is generally regular, with a shape that is neither perfectly round nor highly elongated. No signs of major mergers or significant tidal disturbances are immediately apparent. The galaxy shows a slight asymmetry and potentially a minor disturbance that could be from a small interaction or internal dynamics.
