The galaxy presents as a somewhat elliptical structure, with a smooth, concentrated central bulge. The primary color of the bulge is yellowish-white, suggesting a population of older stars. Extending outwards from the bulge, a faint disk is visible. The disk displays a bluer hue on one side, possibly indicating regions of more recent star formation. There is no clear evidence of spiral arm structure. The overall morphology suggests a galaxy that is transitioning between a spiral and elliptical type. There may be a slight tidal disturbance in the outer disk, which may be the result of a minor merger in its past. The galaxy appears relatively isolated with no clear signs of on-going major mergers or interactions.
