This galaxy appears as a single, concentrated object, suggestive of a relatively smooth morphology. It exhibits a slight elongation, deviating from a perfectly circular form. The color profile indicates a dominant population of older stars, with a central region displaying a yellow-orange hue, possibly indicating an older stellar population. There is a hint of a green-blue halo extending outward, suggesting a possible younger star population. There is no evident spiral structure or strong tidal features to indicate an active merging event, although a mild disturbance cannot be ruled out.
