The galaxy presents as a relatively smooth, somewhat rounded structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There's some evidence of minor disturbances in its overall shape, with a faint suggestion of tidal features or asymmetry, potentially indicating past or ongoing interactions.

The color profile suggests a mix of stellar populations, with a dominant yellowish-red hue in the central regions, indicative of older, cooler stars. Fainter, bluer regions appear marginally, suggesting the presence of younger stars or ongoing star formation in some areas. The overall appearance points to a galaxy that is likely in a transitional phase, possibly evolving from a more actively star-forming state to a more quiescent one.
