The galaxy presents as a relatively small, elongated object with a noticeable degree of internal structure. There is a smooth central bulge which transitions into a more diffuse, extended disk. Within the disk, there appear to be regions of varying luminosity, suggesting non-uniform distribution of stellar populations or dust obscuration. The overall color profile indicates a composite stellar population, exhibiting both bluer regions potentially indicative of younger stars, and redder areas consistent with older stellar populations. There are potential signs of minor tidal features or disturbances extending from the main body of the galaxy, hinting at past or ongoing gravitational interactions. The smooth central component does suggest that a substantial portion of the galaxy's light is emanating from relatively old and undisturbed stars, but the overall distribution of light is somewhat patchy. There is a possible small amount of asymmetry within the galaxy's structure, but this is not a major feature.
