The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular galaxy when viewed from our perspective. The central bulge is prominent and exhibits a higher concentration of light, suggesting a densely populated region of older stars. The light gradually decreases from the center outwards. There is a slight flattening of the galaxy, with its apparent major axis oriented at an angle. No distinct spiral arm structures or prominent dust lanes are visible. Its color index suggests a population of older stars. The light emitted indicates that some star formation may be occurring in the galaxy, albeit at a lower rate relative to typical spiral galaxies. The galaxy appears relatively isolated, without obvious signs of ongoing major mergers or tidal interactions.
