The galaxy presents as a relatively smooth, elliptical object. The light distribution appears centrally concentrated, with a gradual decrease in luminosity moving outward from the core. The color profile is suggestive of an older stellar population, displaying a yellowish-orange hue, which could indicate a lack of significant recent star formation. While there is no clear evidence of spiral arms or a distinct disk structure, there is a hint of bluer regions within the galaxy, which could indicate pockets of younger stars. The overall morphology appears undisturbed, showing no apparent signs of major mergers or tidal distortions, although there are minor disturbances present. There is an indication that the shape of the galaxy is somewhere in between rounded and cigar shaped.
