The galaxy presents as a relatively smooth, elliptical structure. It exhibits a moderate elongation, appearing somewhat cigar-shaped. The core region displays a concentrated, bright, yellowish hue, indicating a likely concentration of older stellar populations. Moving outwards from the core, the galaxy fades into a bluer, less intense halo. There is no prominent evidence of spiral arms or significant dust lanes within the visible spectrum. Based on the smoothness of the galaxy, there do not appear to be any ongoing major mergers. The light distribution suggests the galaxy is likely an early-type galaxy with a significant spheroidal component.
