The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellow-red hue. There is a notable absence of well-defined spiral arms or a prominent disk structure. The overall shape is somewhat elliptical, though deviates slightly from perfect roundness, appearing in between round and elongated. There is no visually apparent ongoing major merger activity or significant tidal disturbance; however, a minor disturbance cannot be ruled out based on the image alone. Judging by the colors and smooth appearance, this galaxy appears to be a relatively evolved system with subdued star formation activity.
