This galaxy presents a concentrated morphology, appearing primarily smooth with a discernible central bulge. The light profile suggests a fairly uniform distribution of stars, with a higher concentration near the core. The overall shape is generally round. A subtle disturbance in the galaxy's form suggests possible interaction with another galaxy or a past minor merger event. The red color suggests that the galaxy consists mostly of older stars with little ongoing star formation. There's no apparent spiral arm structure visible. The galaxy appears to be of significant mass.
