The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars and possibly the presence of an active galactic nucleus, though the image resolution limits definitive confirmation. Moving outward from the core, the luminosity gradually decreases, forming an extended halo. There is some evidence of a slight flattening, indicating that the galaxy is not perfectly spherical but rather somewhat elongated in shape. The overall color appears to be a muted yellowish-white, which implies a stellar population dominated by older, redder stars with limited ongoing star formation. There may be minor disturbances in the shape of the galaxy, perhaps caused by minor gravitational interactions.
