The galaxy presents a generally smooth morphology, with an elliptical shape. The central region exhibits a concentrated, bright core of reddish hue, suggestive of an older stellar population, or significant dust extinction. Moving outwards, the galaxy transitions to a more diffuse, greenish-yellow color, possibly indicating the presence of younger stars and/or emission lines in the spectra, which have been redshifted to appear more green. There appears to be a lack of defined spiral arms or significant substructure, which further supports its classification as a relatively undisturbed, smooth galaxy. Based on color, the galaxy does not appear to have a high rate of star formation. The galaxy is reasonably luminous. No signs of ongoing mergers or major disturbances are readily apparent.
