The galaxy presents as a fairly smooth, centrally concentrated object. The core exhibits a strong, yellowish-white luminosity, suggesting a relatively older stellar population. Surrounding the bright central region is an extended, less intense halo of light. The outer regions of the galaxy fade gradually, with a subtle bluish tint indicating the presence of some younger, star-forming regions. The overall structure appears generally elliptical. There is no readily apparent presence of prominent spiral arms or strong tidal disturbances. The galaxy appears relatively undisturbed, with no indication of ongoing major merging activity.
