The galaxy presents as an elliptical-like structure with a relatively smooth overall appearance. Its central region exhibits a concentrated, bright yellowish-white luminosity, suggestive of an older stellar population. Moving outward from the core, the light profile gradually fades, transitioning to a reddish hue in the outer edges. This color gradient may indicate variations in stellar ages and metallicities, with older, redder stars dominating the outskirts. A slight elongation in the galaxy's shape is discernible. There appears to be a very subtle warp or disturbance in the galaxy's structure.
