The galaxy presents as a somewhat elliptical, relatively smooth structure. The light distribution suggests a centrally concentrated bulge, with a gradual falloff in brightness towards the outer edges. The primary color is a yellowish-white, implying an older stellar population. There are some hints of a faint bluish halo surrounding the main body, which could indicate the presence of younger, hotter stars, but the overall contribution seems minimal. The lack of distinct spiral arms or prominent dust lanes further suggests that this is likely an early-type galaxy, possibly an elliptical or lenticular. The galaxy displays minimal signs of recent mergers or strong tidal interactions, as there are no obvious distortions or extended features around the main body. It exhibits a relatively uniform, stable structure.
