The galaxy presents as a single, relatively smooth structure with a concentrated central bulge. The overall color profile indicates a dominant population of older stars, particularly within the bulge region, showing a yellow-orange hue. The faint, extended halo surrounding the central structure is more subtle and less defined, exhibiting a bluer tint compared to the core. The shape appears mostly elliptical with no discernible spiral arm structures, or any signs of significant tidal disturbances. There may be some minor distortions, but nothing significant. The general appearance indicates a significant fraction of its population of stars is in the early stages of formation.
