The galaxy presents a predominantly smooth morphology, suggesting a likely elliptical classification. The overall shape appears nearly round with a slightly elongated, cigar shaped tendency. The galaxy exhibits a distinct central bulge that displays a concentrated, bright yellowish hue, indicating a population of older stars. The outer regions show a more diffuse glow, transitioning to a cooler color, possibly due to a small amount of younger stars or dust content. There is no clear evidence of spiral arms or significant disk structure. The galaxy appears relatively undisturbed, lacking obvious signs of ongoing mergers or tidal interactions.
