The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse morphology. There is a bright central bulge with a gradual decrease in luminosity towards the outer regions. The color gradient suggests a population of older stars concentrated in the core, indicated by the yellow-orange hue. The outer regions exhibit a bluer tint, potentially indicative of more recent star formation, although this is subdued. The disk appears relatively featureless, with no prominent spiral arm structures visible in this observation. There are hints of slight disturbances in the outer regions, but no major signs of active merging or significant tidal interactions. Overall, the galaxy appears to be an early-type spiral or lenticular galaxy with a relatively quiescent nature.
