The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated, bright central bulge. The light profile fades gradually from the core to the outer regions, with no distinct spiral arm structure visible. The galaxy's color is predominantly yellowish-white, suggesting an older stellar population. Faint reddish features are observable in the outskirts, possibly indicating regions of lower-level star formation or dust. The overall morphology suggests a mature galaxy, likely with a significant spheroidal component. There is no obvious evidence of a major ongoing merger, though some minor disturbance cannot be ruled out due to the faintness of the outer edges.
