The galaxy presents as an elliptical morphology with a smooth appearance. Its central region exhibits a brighter, concentrated luminosity, suggesting a higher density of stellar population or a possible active galactic nucleus. The color profile shows a predominantly bluish-white hue in the central region, transitioning to a redder color in the outer regions. The galaxy appears to be relatively undisturbed, showing no significant signs of tidal interactions or major mergers. Its overall shape is moderately elongated, exhibiting an aspect ratio that deviates from a perfect sphere. There is a slight indication of a disk-like structure within the galaxy, but it is mostly obscured by the smooth, elliptical morphology. There does not appear to be extensive dust lanes or prominent spiral arm features, pointing to a galaxy that has largely exhausted its gas reservoir and has a low rate of star formation.
