The galaxy presents as a relatively smooth, elliptical morphology with a centrally concentrated bulge. The light distribution appears largely homogenous, lacking prominent spiral arm structures or dust lanes. There is a slight elongation to the galaxy's shape, but it appears primarily round. The color profile is generally blue, suggesting the presence of a younger stellar population and ongoing star formation, albeit at a relatively low rate. There are subtle color variations toward the outskirts, with the core region appearing bluer than the surrounding halo. No major merger events are visibly apparent, although there may be some minor disturbances in the outer regions of the galaxy, based on the slightly irregular light distribution. Overall, the galaxy presents as a relatively undisturbed system, likely undergoing a slow, quiescent phase of evolution.
