The galaxy presents as a lenticular or possibly an elliptical galaxy viewed at an oblique angle. It exhibits a smooth, concentrated central bulge which is a bright yellowish-white in color. Surrounding the bulge is a fainter, flattened disk-like structure, also yellowish, suggesting an older stellar population with minimal ongoing star formation. The galaxy appears largely undisturbed with no obvious signs of major mergers or tidal interactions. It is elongated, appearing cigar-shaped rather than perfectly circular, which could result from its intrinsic shape or viewing angle. There is a subtle color gradient across the galaxy, with the central bulge being slightly more yellow than the outer regions, potentially indicative of differences in stellar population ages and metallicities. The overall morphology suggests a relatively massive galaxy, evolved in structure and dominated by older stars.
