The galaxy presents as a somewhat elliptical, though not perfectly round, structure. It exhibits a central, concentrated bulge of light that appears to be a yellowish-white hue, indicative of a population of older stars. The outer regions of the galaxy are less defined, with a more diffuse, blue-tinged glow suggesting the presence of some younger, hotter stars, though they do not dominate the stellar population. There is a very slight hint of disturbance on one edge, it does not appear to be undergoing a major merger event, but there might be some minor tidal interaction occurring. Overall, the galaxy appears to be a relatively smooth system, without prominent spiral arms or strong irregularities.
