This galaxy presents as a somewhat elliptical or disk-like structure, although not perfectly symmetrical. The central region exhibits a noticeable concentration of light, appearing brighter and more intense than the outer regions. The light appears redder in the center as well. The outer regions appear more diffuse and spread out, with a faint greenish tint. There is no visible spiral structure or distinct features, suggesting a relatively smooth morphology. Evidence indicates only minor disturbances from possible gravitational interaction or past mergers. Overall, the galaxy appears relatively isolated and not currently undergoing any major interaction with other galaxies.
