The galaxy presents as a relatively smooth object, exhibiting an elliptical morphology with a slight elongation. The central region displays a brighter, concentrated luminosity profile, suggestive of a significant stellar population density or possible active galactic nucleus. A fainter, more diffuse halo or extended envelope surrounds the central region, gradually fading into the background sky. There is subtle color variation across the galaxy, with a generally bluer hue in the outer regions, possibly indicating the presence of younger stellar populations or ongoing star formation, while the central regions appear somewhat redder, which would align with an older, more evolved stellar population. No distinct spiral arms or prominent dust lanes are discernible from the image. There is some evidence of a very slight minor disturbance in the galaxy's shape. Overall, the galaxy appears as a relatively undisturbed, mature system.
