The galaxy presents as a relatively smooth and concentrated structure. The central bulge region is noticeably bright, exhibiting a yellowish hue. It exhibits an elliptical morphology, with a generally rounded shape but with some deviation from perfect circularity. There is a lack of distinct spiral arm structure or prominent dust lanes visible. The galaxy appears to be relatively isolated, showing no signs of ongoing major mergers or strong tidal disturbances. A hint of a more diffuse outer halo surrounds the central region, though its boundaries are indistinct. Star formation seems to be low as there are no bright blue regions from new stars.
