The galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated shape. The central region exhibits a bright, concentrated luminosity, suggesting a high density of stars and possibly an active galactic nucleus, though further spectroscopic data would be needed to confirm the presence of an AGN. The galaxy's color is predominantly reddish-orange, indicative of an older stellar population with fewer young, blue stars. There is little evidence of prominent spiral arms or significant dust lanes. A faint, diffuse halo extends outwards from the central region. There is no apparent interaction or disturbance from nearby galaxies to suggest a merger is taking place.
