The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The central region exhibits a bright, diffuse glow, indicative of a high stellar density. Moving outward, the light gradually fades into a less luminous halo. The galaxy's shape appears to be elongated, deviating slightly from a perfect sphere. There is an apparent lack of distinct spiral arms or prominent dust lanes, consistent with an older stellar population. Subtle color gradients are present, with a redder hue concentrated in the core, potentially suggesting an increased presence of older, redder stars, and a bluer, more diffuse glow further from the center. The overall structure suggests a relatively evolved system, likely dominated by older stars with little ongoing major star formation. There appears to be evidence of a minor tidal disturbance, evidenced by slight asymmetry in the outskirts, potentially indicative of a past or ongoing minor merger event. 
