The galaxy presents as a relatively smooth, elliptical structure, exhibiting a central bulge that is bright and somewhat elongated. The color gradient suggests a concentration of older stellar populations in the core, shifting to a slightly bluer hue in the outer regions. There is no discernible spiral arm structure or prominent dust lanes. The galaxy appears to be a nearly edge-on disk, with the major axis longer than the minor axis. There is an apparent absence of major tidal disturbances or close companion galaxies that might indicate an ongoing or recent merger event, though the asymmetry could indicate a past minor merger. Overall, the galaxy appears to be a relatively evolved system with a modest amount of ongoing star formation.
