The galaxy presents as a relatively smooth, elliptical-like structure, appearing elongated with a cigar shape morphology. A bright, concentrated central bulge is observed, gradually fading outward into a more diffuse halo. The overall color appears to be a bluish-white hue, with a subtle gradient from the core outwards. There is no apparent evidence of prominent spiral arms or dust lanes. Indications of a minor disturbance are present, but overall the galaxy appears relatively isolated and undisturbed. Star formation activity appears to be low.
