The galaxy presents as a moderately small, elongated structure with a smooth, diffuse appearance. It exhibits a subtle color gradient, appearing slightly bluer at one end, which could be indicative of localized star formation activity. The overall form suggests either an elliptical galaxy viewed along its major axis, or potentially a highly inclined spiral galaxy where the disk structure is not readily apparent. There is no clear evidence of a prominent nucleus or distinct spiral arms, but a subtle central condensation might be present. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
