The galaxy presents as a single, concentrated object with a smooth, rounded appearance. The light distribution suggests a dominant central bulge with a relatively small disk or halo component. It exhibits a yellowish-white color, suggestive of an older stellar population and lower levels of ongoing star formation. There is no evidence of spiral arms, bar structures, or any significant morphological disturbances, such as tidal tails or interacting companions. The galaxy appears to be relatively undisturbed and shows no signs of recent or ongoing merger activity. It is unresolved and compact.
