The galaxy presents as a luminous, disk-shaped structure. The central region exhibits a concentrated, bright yellowish-white hue, suggesting a high density of older stellar populations. Moving outward from the core, the disk displays a subtle transition towards a slightly redder tint. A faint blue-green arm appears in the central region. The overall smoothness of the light distribution implies that the stellar population is well mixed. The galaxy appears to have a relatively compact morphology with a shape that can best be described as somewhere between round and cigar-shaped. There is no visible evidence of major disturbances or ongoing merger activity.