The galaxy presents as a relatively smooth, single structure, seemingly elliptical in shape, although a minor irregularity in the disk hints at a possible past interaction. The color gradient shifts from a warmer, yellowish central region to cooler, redder outer edges, which indicates an older stellar population dominates the core, while the outer regions might have a lower average stellar age or be more dust-reddened. There's no obvious spiral structure, and the light is centrally concentrated. A faint, diffuse halo is suspected, but its extent and properties are difficult to discern given the image resolution. The galaxy's overall morphology suggests it is not undergoing any major mergers at this time, and no significant tidal features are observed, however there is an object which seems to be very close to merging, which is causing some disturbance in the shape. The light profile appears consistent with an evolved galaxy dominated by older stars.