The galaxy appears to be an elliptical type, exhibiting a largely smooth and featureless morphology. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer edges. The shape is somewhat elongated, tending towards a cigar-like form rather than perfectly circular. There is no apparent evidence of a spiral arm structure or a prominent disk component. The color profile suggests a relatively old stellar population, with a yellowish-white hue at the core transitioning to a bluer tint towards the periphery. There are no visible signs of major mergers or tidal disturbances, though a possible minor disturbance cannot be ruled out. Overall, the galaxy presents as a relatively undisturbed system, consistent with a mature elliptical morphology.
