The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The overall color appears slightly yellowish, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The morphology indicates a system with minimal ongoing star formation and a dominant, well-established stellar population. The galaxy exhibits a slight elongation in its shape, but does not appear heavily distorted. There is no strong indication of an active galactic nucleus or recent merger events affecting the system's structure. The object appears relatively undisturbed.
