The galaxy appears as a diffuse, moderately luminous object. It exhibits a somewhat elliptical morphology, lacking any distinct spiral arm structure. There is a noticeable concentration of light towards the central region, suggesting the presence of a bright galactic nucleus. The overall color appears to be relatively uniform across the galaxy, with a slight yellowish hue. This coloration suggests a population of older stars. There is some subtle asymmetry in the outer regions, potentially indicating minor gravitational disturbances or interactions with smaller satellite galaxies. 
