The galaxy presents as a moderately luminous, relatively smooth object with a slightly elongated, disk-like appearance. It exhibits a concentrated central bulge region which appears largely featureless. The color profile suggests a dominant population of older stars, with a notable absence of significant blue emission indicative of recent, intense star formation. There are some subtle disturbances or features in the outer regions of the galaxy which may indicate some minor mergers or tidal interactions. Its overall structure appears relatively undisturbed, with no obvious signs of ongoing major mergers or significant tidal disruption. The object is mostly round.
