This galaxy presents as a relatively smooth, centrally concentrated object with a mild degree of ellipticity. The core appears to be dominated by older stellar populations, indicated by the yellowish-orange hue. Moving outwards from the center, the galaxy exhibits a gradual decrease in surface brightness. There is a subtle color gradient, with bluer tones becoming slightly more prevalent in the outer regions, suggestive of some ongoing star formation. The overall structure indicates that this galaxy is not currently undergoing any major merging activity, however, there are some minor asymmetrical features suggesting there may be some internal dynamics. The galaxy's morphology is largely consistent with that of an early-type galaxy, possibly an elliptical or lenticular galaxy. 
