The galaxy presents a generally elliptical morphology, appearing cigar-shaped. The central bulge exhibits a high degree of smoothness, with a concentrated luminosity gradient. The outer regions show a gradual decline in surface brightness, with subtle indications of a disk-like structure. There appears to be no substantial dust lane obscuring the central regions. The overall color index indicates a more evolved stellar population, with a yellowish-red hue. No prominent spiral arms or active star-forming regions are readily apparent. There are signs of possible minor disturbances.
