The galaxy presents as an elliptical or spheroidal system. The light distribution is centrally concentrated with a smooth profile, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits a yellowish-red color, suggesting a population of older stars and a lower rate of ongoing star formation, potentially indicative of a more evolved system. It appears relatively isolated, showing no strong signs of tidal disruption or interaction with other galaxies. The object displays a compact morphology with an estimated radius of approximately 3 kpc. There is little dust.
