The galaxy presents as an elongated, disk-like structure viewed at an oblique angle. Its central region exhibits a concentrated, bright yellowish-orange glow, suggestive of an older stellar population or significant dust obscuration. The outer regions of the disk are less defined, appearing fainter and somewhat blurred, with a bluer hue compared to the core. The overall shape appears relatively smooth, with no obvious signs of major tidal disturbances or ongoing mergers. A slight asymmetry may be present in the outer disk. The galaxy’s morphology appears to be that of a spiral or lenticular galaxy, with the suggestion of a thin disk. There does not appear to be any recent activity based on the smooth gradient to the bluer outer regions. 
