The galaxy presents a largely smooth and round morphology. There is a distinct central bulge with a yellowish-orange hue, indicative of an older stellar population. Surrounding this bulge is a fainter, more diffuse halo of light with a slightly bluer tint, suggesting the presence of younger stars, however there does not appear to be a significant amount of ongoing star formation. It is possible there is a disk, but it is not well defined. There are no obvious signs of spiral arms, bars, or significant dust lanes within the observed structure. The galaxy appears relatively isolated, with no immediate signs of tidal interactions or ongoing mergers.
