The galaxy presents as a relatively smooth, elliptical or lenticular system. The core exhibits a concentrated, bright luminosity, possibly indicative of an active galactic nucleus or a dense stellar population. The light is heavily concentrated, with a slightly out-of-round, elliptical shape. Some of the light is yellow-tinged, which can be indicative of a slightly older stellar population compared to typical spiral galaxies, in which younger blue stars are more common. A small, diffuse halo of lower surface brightness light extends beyond the core, suggesting the presence of older stars in the outer regions. There are no spiral arm structures visible. No significant dust lanes or signs of ongoing major star formation activity are apparent. Overall, the galaxy's morphology suggests a relatively evolved system.
