The galaxy presents as a generally smooth, elliptical morphology. It exhibits a notable radial color gradient, transitioning from a concentrated, redder core to a bluer, more diffuse outer halo. The central region shows a high degree of symmetry and lacks any immediately apparent dust lanes or distinct spiral arm structures. There is a slight elongation present, but overall the shape approximates a spheroid. While appearing largely undisturbed, a very faint, asymmetrical feature is detectable in the outer regions, potentially suggestive of a minor tidal interaction or past merger event, although this is not definitive from the image alone. There is a detectable amount of ongoing star formation, given the galaxy's blue color, with most of it concentrated in the outskirts of the galaxy. 
