The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile appears to gradually decrease in intensity from the core outwards, lacking any prominent spiral arm structures or significant dust lane features. The shape is more elliptical than circular, but not highly elongated; it appears to be an intermediate elliptical shape. The dominant color is a yellowish-orange hue, suggestive of an older stellar population. There is a subtle color gradient, with the central region appearing slightly more yellow, potentially indicating a higher concentration of older, redder stars or a lower rate of recent star formation. There is no readily apparent evidence of ongoing mergers or tidal disturbances in the immediate vicinity. The overall impression is of a galaxy that is relatively quiescent and evolved.
