The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that fades gradually into the surrounding halo. The core displays a yellowish hue, indicative of an older stellar population. The galaxy appears fairly round in shape with a slight deviation from perfect circularity. There is no discernible spiral arm structure or prominent dust lanes. The overall luminosity suggests it is a relatively massive galaxy. There is no apparent evidence of a major merger or significant tidal disturbances. Star formation is likely occurring at a low rate.
