The galaxy presents a largely smooth morphology, exhibiting a high degree of radial symmetry. Its shape is primarily round. The central region displays a bright, concentrated core, suggesting a substantial stellar density. The color profile indicates a redder hue, implying a population dominated by older stars. There is very little evidence of spiral arm structure or significant dust lanes. Minimal tidal features are observed, suggesting it is unlikely undergoing a major merger event. Subtle irregularities in the outer regions might indicate minor disturbances, possibly from past interactions. Overall, the galaxy appears to be a relatively quiescent system.
