The galaxy presents a roughly elliptical morphology, exhibiting a diffuse, unresolved structure. A central bulge is discernible, appearing brighter and more concentrated than the surrounding galactic disk or halo. The overall color profile suggests a generally older stellar population, although some bluer hues are present, particularly in the outer regions, potentially indicating ongoing or recent star formation activity. Faint tidal features or asymmetries are visible which might indicate a recent or ongoing minor merger event or gravitational interaction. There appears to be no well-defined spiral arm structure observable in this image.
