The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The color index suggests a population dominated by older, redder stars. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears quite round, lacking a strongly elongated or cigar-shaped appearance. There is no obvious evidence of recent or ongoing major merger activity, though there is a smaller object nearby on the right of the image that could be interacting with it. Based on its color and morphology, the galaxy is likely an early-type galaxy, with a relatively low rate of star formation.