The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core region exhibits a bright, yellowish-white glow, suggesting a population of older stars. There appears to be a very subtle, diffuse disk component, though the dominant morphology is that of a spheroid. No prominent spiral arms or distinct star-forming regions are discernible within the visible light bands, implying a low current star formation rate. The overall color profile indicates a relatively evolved stellar population. There is no obvious tidal disruption or interaction with other galaxies in the immediate vicinity. The shape is very round, with hints of oblateness.
