The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. The color profile suggests a red core with a faint, diffuse, greenish halo extending outwards. There is minimal evidence of spiral arm structure or significant dust lanes. The overall appearance indicates a system dominated by older stellar populations, with a relatively low ongoing star formation rate. There is a slight elongation of the galaxy, but it appears mostly symmetrical without significant tidal disturbances or signs of a major merger event. Minor asymmetry is present, possibly indicative of a minor interaction or internal processes.
