The galaxy appears to be a relatively compact object with a smooth, elliptical morphology. There is little evidence of significant spiral arm structure or prominent dust lanes. The light distribution suggests a central concentration with a gradual decrease in brightness towards the outer regions. The color profile seems rather homogenous across the galaxy, dominated by yellowish-white hues, which may indicate an older stellar population with lower levels of current star formation. The galaxy's round shape and smooth appearance suggests that it is likely an early-type galaxy. The slight asymmetry in the outer edges indicates a very slight possibility of an interaction or minor disturbance. However, the overall structure implies that the galaxy is largely undisturbed and relatively isolated.
