The galaxy presents a mostly smooth, rounded morphology, suggesting an elliptical or lenticular classification. The light distribution indicates a centrally concentrated bulge component, gradually fading outwards. There is little indication of spiral arms or significant disk structure. The color gradient shifts from slightly bluer hues in the central region towards redder hues in the outer parts. This could be indicative of an older stellar population in the outer halo, with some ongoing star formation in the core. Overall, the galaxy does not appear to be significantly disturbed, with no signs of major mergers or tidal features visible in this image. However, there may be some minor disturbance or interaction.
