The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge with a noticeable, though subtle, color gradient transitioning from a yellowish core to slightly bluer outer regions. The overall shape is largely spheroidal with no obvious disk-like structures or spiral arms visible at this resolution. There is little evidence of significant star formation within the galaxy, with the yellow hue of the core indicating an older stellar population. No signs of a major ongoing merger are immediately apparent, though there might be subtle indications of minor disturbances in the galaxy's outer regions.
