The galaxy presents as a moderately bright, elliptical morphology. A central bulge dominates the luminosity profile, exhibiting a smooth, diffuse appearance with a yellowish hue. The isophotes appear elliptical, with the major axis oriented at approximately 60 degrees from the vertical. There is a gradual decrease in surface brightness moving outwards from the central bulge, with no distinct spiral arm structures visible. The outer regions exhibit a bluer color than the core, possibly indicating the presence of younger stellar populations there. The overall structure is relatively smooth with only a slight hint of asymmetry, perhaps indicating a minor gravitational interaction or past merger event. No strong dust lanes or prominent star-forming regions are immediately apparent in the image.
