The galaxy presents as a single, relatively smooth, centrally concentrated object. It exhibits an approximately elliptical morphology. The galaxy's core appears luminous with a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a more diffuse and slightly bluer shade, implying the potential presence of younger stars or ongoing star formation, albeit at a lower rate. There is no distinct disk structure or spiral arm features visible in this observation. There might be slight distortions or minor disturbances in the outer regions, though they don't appear to be indicative of a major ongoing merger. The overall appearance indicates a system that is relatively settled, leaning toward an elliptical or lenticular classification.
