The galaxy presents a predominantly smooth, elliptical morphology, exhibiting a concentrated central bulge. The light distribution appears relatively uniform across the main body of the galaxy, indicative of an older stellar population. There is a slight deviation from perfect circularity, but the overall shape approximates a spheroid. The color appears to be yellowish-red, suggesting a lack of significant ongoing star formation. A faint blue region is visible along one edge, which could indicate a region of younger stars, a tidal feature, or background/foreground galaxy. There is no readily apparent disk structure or spiral arms, and no significant dust lanes are discernible. There is no evidence of a major ongoing merger or strong tidal interactions.
