The galaxy presents as a somewhat elliptical object. The central region appears as a bright, concentrated bulge, likely dominated by older stellar populations. The color gradient transitions from a bluer core to redder outer regions, suggesting ongoing or recent star formation closer to the center with a decrease towards the outskirts. Faint, diffuse features extend outwards from the central bulge, but these are not well-defined spiral arms or a distinct disk structure. Overall the galaxy appears relatively undisturbed morphologically, with only minor evidence of tidal features that could be attributed to minor interactions. The shape is relatively in between, not clearly defined in any particular shape category.
