The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is noticeably brighter than the surrounding areas. The color profile suggests a population of older stars, with a general yellowish-red hue dominating, although a slight bluer tinge is also visible across the disk. There is a general absence of prominent spiral arm structures or distinct dust lanes. The overall morphology indicates a fairly relaxed system, with only subtle disturbances observed in the outer regions.
