The galaxy presents as an elliptical or lenticular system, exhibiting a relatively smooth, featureless morphology. It appears elongated with a pronounced bulge. The core of the galaxy shows a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. There are hints of a faint, diffuse halo surrounding the central region. The overall color indices suggest a population of older stars, with a lower rate of ongoing star formation. No distinct spiral arms or dust lanes are discernible. The system may be exhibiting minor gravitational interactions.
