The galaxy presents as a single, somewhat elliptical object. The light distribution appears centrally concentrated, with a bright core that gradually fades outward. The galaxy exhibits a smooth morphology without any prominent spiral arms or distinct features, like dust lanes. There is a slight elongation in the shape, suggesting it is not perfectly spherical. The galaxy appears relatively isolated, without obvious signs of ongoing major merging or tidal disturbances in its immediate surrounding field. The color profile seems to have a moderate red tint, potentially indicating an older stellar population or the presence of dust.
