The galaxy presents as a single, largely featureless object. It exhibits a concentrated central bulge, brighter and yellower than the surrounding regions, which suggests a higher density of older stars in this area. The outer regions appear somewhat less concentrated and diffuse. The overall shape is mostly round and smooth. There is no apparent disk structure or spiral arms. The color appears to be a mix of yellow and red hues, with the core tending towards the yellow end of the spectrum. This would generally indicate a lower rate of star formation across the entire galaxy. There seems to be no major merging event disrupting the shape of the galaxy. There may be a minor perturbation event happening, though no visible disturbances are present.
