The galaxy exhibits a generally elliptical morphology, though some asymmetrical features are present. A bright, concentrated central bulge dominates the structure, appearing yellowish-orange in color, suggesting a population of older stars. The surrounding disk or halo is less defined, displaying a fainter and bluer color profile. There is evidence of a potential spiral arm or tidal feature extending outward from the main body on one side of the galaxy, showing some signs of recent star formation. The overall structure appears somewhat disturbed, possibly indicative of a past or ongoing interaction or merger event.
