The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spherical and intensely luminous, likely indicative of a concentrated stellar population. The luminosity decreases gradually towards the outer regions, but lacks distinct spiral arm structures or a prominent disk. There is a slight elongation, but the overall shape is closer to circular than cigar-shaped. No major disturbances or mergers are visually apparent, with a relatively undisturbed structure. The galaxy exhibits a blueish hue, potentially suggesting moderate star formation activity, although the smoothness indicates an older stellar population is also present.
