The galaxy presents as an elliptical morphology, exhibiting a smooth, diffused light distribution with a high degree of central concentration. The shape is somewhat elongated, approaching a cigar-like appearance. There is no clear evidence of spiral arms, dust lanes, or a prominent galactic disk. The color is generally yellowish-white, suggesting a stellar population dominated by older stars. The overall structure appears relatively undisturbed, with no strong indications of ongoing or recent major mergers or tidal interactions. Minor disturbances cannot be ruled out entirely, but the dominant impression is that of a relaxed system.
