The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated core region dominates the galaxy's structure, indicating a high stellar density in the central region. Surrounding this core is a more diffuse, extended halo. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape, but is closer to round than cigar-shaped. There is no prominent disk structure apparent. There is a slight disturbance from a nearby source, but no major signs of ongoing mergers or significant tidal interactions are visible. Overall, the galaxy appears to be a relatively undisturbed, evolved system with a dominant spheroidal component.
