The galaxy presents as a relatively smooth, disc-shaped structure. It exhibits a central bulge that appears more luminous than the surrounding disc, suggesting a higher concentration of older stars in this region. The overall color is somewhat redder, indicating a stellar population that is not dominated by young, blue stars. The galaxy is elongated, but not extremely so, with no obvious spiral arm structure visible. There is no strong evidence of recent or ongoing major mergers or interactions with other galaxies. The disk appears relatively undisturbed with no apparent major distortions or tidal features. The galaxy appears to be in a relatively quiescent state, with a low rate of star formation.
