The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a notable central bulge. The galaxy's color profile suggests an aging stellar population, with a predominantly yellow-red hue indicating a lack of significant ongoing star formation. There is minimal evidence of spiral arms or disk-like structures. The light appears to be evenly distributed, suggesting an older system. The galaxy displays a somewhat round shape, with only slight elongation. There does not seem to be evidence of recent or ongoing merging activity or major disturbances. The galaxy's size is relatively compact.