The galaxy appears to be an elliptical galaxy, characterized by a relatively smooth, featureless appearance. It exhibits a somewhat elongated, cigar-like shape. The color distribution suggests a dominant population of older stars, indicated by the reddish hues, particularly in the central bulge. There is some evidence of bluer light indicative of younger stars. There is a minimal indication of spiral arm structure, indicating a galaxy that is smooth or has had its spiral structure disrupted. There are no obvious signs of major mergers or tidal disturbances, though subtle minor disturbances may be present. 