The galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy given its apparent lack of spiral arms or prominent disk structures. There is a distinct, diffuse central bulge with a noticeable color gradient, transitioning from a slightly redder hue in the core to a bluer tint towards the outer regions. This could indicate a centrally concentrated population of older, redder stars, potentially surrounded by a younger stellar population or regions of ongoing star formation. The galaxy does not display any obvious signs of major mergers or significant tidal disturbances, but a subtle asymmetry or minor irregularity in the outer isophotes cannot be ruled out at this resolution. Overall, the galaxy presents as a fairly undisturbed system, appearing mostly round and showing no characteristics indicative of a significant disk.
