The galaxy appears as a somewhat diffuse, luminous object with an elliptical shape, possibly undergoing a merging event. The color gradient suggests a relatively evolved stellar population, with a concentration of older, redder stars dominating the central region. There are subtle hints of disruption in the galaxy's morphology, possibly indicative of tidal interactions or recent merger activity. While there's no clear presence of distinct spiral arms, some faint bluer regions may indicate ongoing star formation. Overall, the galaxy shows signs of both mature stellar components and localized regions of younger stars, potentially influenced by its dynamical state.
