The galaxy appears as a centrally concentrated, smooth object. Its overall shape is elliptical, tending towards a rounded morphology, with no clear presence of a disk. The color profile suggests a moderate population of older stars, with a possible presence of ongoing, but limited, star formation. There is no strong evidence of spiral arms or other distinct features within the galaxy. No major disturbances due to galaxy mergers appear to be visibly affecting the overall structure. The light profile indicates the galaxy is relatively compact. The object's color is slightly more intense in redder wavelengths and less so in bluer wavelengths.
