The galaxy presents a largely smooth, elliptical morphology. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy's light profile exhibits a strong central concentration, with a gradual decrease in intensity moving outwards from the core. The galaxy's color appears relatively uniform, with a slight reddish-yellow hue indicative of an older stellar population, though this could also be caused by redshift. There are no obvious signs of a major ongoing merger or strong tidal disturbances. The overall appearance suggests a well-evolved system with a relatively quiescent star formation rate. The object is fairly compact and shows a degree of roundness, with no strong elongation or bar-like feature visible. Any substructure is very subtle and not easily discernible within the limits of the image resolution.
