The galaxy presents as a centrally concentrated, elliptical morphology. The light distribution is smooth, with a high degree of radial symmetry. A bright, compact core is apparent, indicative of a spheroidal structure with a concentration of older stars. The galaxy has an average size of about 6 kpc. The color appears to be a yellowish-red hue, suggesting an evolved stellar population and a relatively low rate of ongoing star formation. There's no strong visual evidence of spiral arms or significant dust lanes. No major merging or tidal disturbances are apparent, though very minor distortions cannot be ruled out. The galaxy appears relatively isolated.