The galaxy presents a primarily smooth morphology, with a subtle elongation suggesting an elliptical or lenticular classification. There is a faint disk-like structure that is difficult to distinguish. Its central bulge exhibits a higher surface brightness than the outer regions. The color profile suggests a population of older stars, with a reddish hue. While it appears largely undisturbed, there is a slight asymmetry which hints at a possible minor interaction or past merger event. Overall, the galaxy is relatively compact and likely possesses a moderate mass. The star formation rate seems to be quite low.