The galaxy presents a generally smooth, elliptical morphology. The core exhibits a high degree of central concentration, with luminosity decreasing gradually towards the outer regions. There is a slight elongation, deviating from a perfectly circular shape, tending towards a more flattened or "in-between" rounded appearance. Faint hints of disc-like features are observed. There is no indication of ongoing major mergers or significant tidal disturbances; any potential interactions appear to be minimal. Color gradients are subtle, the central region displays a yellower hue suggestive of an older stellar population, while the outer regions appear marginally bluer, possibly indicating pockets of younger stars or residual star formation. The galaxy is of intermediate size for objects of this type. Overall, the galaxy appears to be a relatively evolved system with a dominant spheroidal component.
