The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. A bright, yellowish core dominates the light profile, suggesting a significant population of older stars or the presence of an active galactic nucleus. The outer regions of the galaxy exhibit a faint, diffuse halo with hints of a subtle disk-like structure. The overall color indices appear to be redder, consistent with a galaxy containing a significant fraction of evolved stellar populations and relatively low current star formation activity. There is no obvious evidence of significant tidal features, major mergers or strong disturbances within the galaxy. Some slight indications of minor disturbances exist with possible faint irregularities in the outer halo.
