The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated luminosity profile. The core appears bright and diffuse, gradually fading outwards into the surrounding halo. There is a subtle color gradient, trending towards redder hues in the central regions and a slight bluer tint towards the outer edges. No distinct spiral arms or prominent dust lanes are discernible. The galaxy exhibits a near-circular shape with a slight elongation. There is no evidence of active galactic nuclei activity or recent major merger events. The overall appearance suggests a relatively evolved system dominated by an older stellar population.
