The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is brighter and has a yellow/orange hue, suggesting an older stellar population. The overall form is somewhat rounded but appears to be slightly elongated. There is little to no visual evidence of spiral arms or a distinct disk structure. A faint halo surrounds the central region, gradually fading into the background sky. No major disturbances or merging features are readily apparent, although subtle asymmetries or tidal tails cannot be completely ruled out at this resolution. The light distribution suggests a relatively quiescent galaxy with a dominant spheroid component.
