The galaxy presents as a generally smooth and rounded structure, with a highly concentrated central bulge. The light profile appears relatively uniform, fading gradually towards the outer edges, indicating a lack of distinct spiral arms or prominent features. A color gradient is discernible, with the central region exhibiting a yellowish-white hue, suggesting a population of older stars. The outer regions display a bluer tint, implying the presence of a younger stellar population or ongoing star formation, albeit at a seemingly low rate. There is no evidence of significant tidal disturbances or mergers; the overall morphology suggests a relaxed, relatively undisturbed system.
