The galaxy presents as a relatively well-defined elliptical shape, with a smooth, concentrated light profile. Its core region appears very bright and unresolved, suggesting a significant concentration of older stars or a possible active galactic nucleus, though the resolution limits definitive determination. The surrounding disk exhibits a somewhat hazy, diffuse structure, possibly indicative of ongoing star formation, dust, or a fainter, more extended stellar population. The color gradient shows a shift from bluer hues at the outer edges to a slightly redder color toward the center. There are some subtle irregularities visible in the disk, implying potential minor disturbances or interactions, although no clear merger events are apparent. The overall morphology suggests a mature galaxy, likely in the process of transitioning from star formation to a more quiescent state.
