The galaxy presents an elliptical morphology, appearing primarily smooth with a bright, concentrated central bulge. Faint disk-like structures may exist but are difficult to assess given the viewing angle and resolution. Some disturbances appear to be present in the galaxy's structure, possibly indicative of a minor merger event in progress, or a recent past interaction. The light distribution suggests a gradual falloff in intensity from the core towards the outer regions. There is a small hint of bluer colorations on the edges, though the predominant color is reddish. The overall features suggest a galaxy evolving through the red sequence.