The galaxy presents an elongated, cigar-shaped morphology, with a smooth, centrally concentrated bulge exhibiting a yellowish hue. The overall color suggests a stellar population dominated by older stars. There is a slight disk-like structure observed, but no prominent spiral arms.  The galaxy appears relatively undisturbed, showing no strong evidence of recent major mergers or tidal interactions, though there is a slight asymmetry that could indicate a minor disturbance event. Star formation appears to be relatively low.
