The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core. A faint, diffuse halo surrounds the core, fading into the background. There is some possible evidence of a slight distortion or tidal feature, but it is not clear. The color profile suggests the presence of older stellar populations. There are very few star forming regions evident in the images. The galaxy appears relatively isolated and is likely a mature system.
