The galaxy presents a primarily smooth, elliptical morphology. There is a distinct central bulge exhibiting a concentrated, bright yellowish hue, suggestive of an older stellar population. This transitions into a less concentrated, slightly bluer halo surrounding the core. This halo shows hints of disk-like features, although no distinct spiral arms are discernible. The overall shape is intermediate between round and elongated, with a slight cigar-shaped deviation. There is no clear evidence of a major ongoing merger or significant tidal disturbances, although some minor asymmetry and faint extensions from the main body could suggest subtle interactions or minor disturbances. The estimated size suggests a moderately large galaxy. The color gradient, from yellow to a pale blue moving outwards, may indicate ongoing star formation in the outer regions, though the overall smooth appearance suggests a relatively passive galaxy.
