The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology indicates a primarily spheroidal structure, displaying a high degree of roundness. There is minimal indication of a prominent disk component or significant spiral arm structure. No signs of active galactic nuclei or jet emission can be seen from this image. The red color of the galaxy suggests a population dominated by older stars, which is consistent with a low star formation rate. There is no sign of gravitational interaction or tidal disruption, which could suggest a recent or ongoing merger. The galaxy exhibits a redder color, potentially reflecting an older stellar population. Overall, the galaxy presents a fairly undisturbed, evolved system.
