The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, diffuse light profile, with a notable absence of distinct spiral arms or prominent features. The core region shows a bright, concentrated luminosity, transitioning gradually outward to a fainter halo. The overall color is a warm yellow-white, suggesting a stellar population dominated by older, evolved stars. The aspect ratio indicates a slightly elongated shape, but the galaxy does not appear to be highly flattened. There is no readily apparent evidence of ongoing major mergers or significant tidal disturbances. Faint, subtle irregularities or extensions in the outer regions cannot be entirely ruled out, but the dominant impression is one of a relaxed, mature system.
