The galaxy presents as an elliptical morphology, appearing largely featureless with a high degree of central concentration. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. Fainter, bluer light extends from the center, possibly indicative of some ongoing star formation. There is no apparent spiral arm structure or significant dust lane obscuration. The overall smooth appearance points towards a galaxy that has largely completed its major mergers and is in a relatively quiescent state. Minor asymmetries cannot be ruled out, but the galaxy is primarily a relaxed, spheroidal system.
