The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. The overall color appears reddish-yellow, with a gradual fading towards the outer edges. There is a slight asymmetry that can be observed but it does not have a well defined disk or spiral arms. The morphology suggests a lack of significant recent mergers, though possible minor disturbances are suggested by slight irregularities in the outer halo. The red color implies a population of older stars and a relatively low rate of ongoing star formation within the galaxy, though the inner yellow light indicates that some active stars are still present within the galaxy. Based on the observed characteristics, the galaxy appears to be a massive system that has not had a major merger recently. 
