The galaxy appears to be relatively compact, showing a smooth, elliptical morphology. There is a noticeable bulge component with a gradual decrease in luminosity toward its outer regions. The light distribution suggests an absence of significant spiral arm structure or prominent dust lanes. The overall color is moderately blueish, which could suggest the presence of some ongoing, though perhaps not intense, star formation. There does not appear to be evidence of strong tidal features or major mergers, though some minor disturbances cannot be entirely ruled out at this resolution. The galaxy exhibits a slight deviation from perfect circularity, appearing somewhat elongated or oval in shape.
