The galaxy presents as a relatively smooth, elliptical-like object with a noticeable central bulge. The primary color is yellowish-white, suggesting an older stellar population and a relative lack of ongoing star formation. Fainter blue emissions can be observed in a somewhat ring-like structure extending radially outwards, possibly hinting at a limited amount of star formation in the outer regions. There is no visible evidence of spiral arm structure or significant dust lanes. The galaxy appears to be isolated, with no obvious signs of tidal interactions or ongoing mergers.
