The galaxy appears as a slightly elongated, diffuse structure with a smooth morphology. Its central region exhibits a concentrated brightness, suggesting a bulge component. There is a lack of distinct spiral arms or prominent dust lanes visible in this image. The overall color profile is slightly yellowish, which could indicate a population of older stars and/or moderate dust obscuration. There are potential signs of minor gravitational disturbance occurring within the galaxy. The size of the galaxy is relatively substantial.
