The galaxy presents as an elliptical or lenticular type, characterized by a generally smooth, featureless appearance and a centrally concentrated light profile. It is yellowish with a slight green tinge. There is no visible spiral arm structure or dust lane obscuration. The galaxy exhibits a high degree of symmetry, lacking any obvious distortions or tidal features, suggesting it is not currently undergoing a major merger. The central region appears brighter and more intensely yellow than the outer regions, possibly indicating a higher concentration of older stars, or potentially emission from a weak active galactic nucleus. It is an isolated galaxy with a somewhat round shape.
