The galaxy presents as a relatively smooth, elliptical structure. The light distribution appears concentrated towards the center, with a gradual decrease in intensity extending outwards, giving it a somewhat elongated, cigar-like shape. There is little evidence of spiral arms or prominent dust lanes. The primary color appears to be slightly reddish, suggesting an older stellar population and minimal ongoing star formation. There is no obvious indication of a recent or ongoing major merger event, although some minor disturbances or tidal features cannot be ruled out at this resolution. Overall, the morphology suggests a galaxy that is relatively evolved and quiescent.
