The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in luminosity as the radius increases. The color gradient suggests an older stellar population, with a yellowish-white hue dominating the central regions. The galaxy's shape is elongated, appearing somewhat cigar-shaped rather than perfectly spherical. No clear signs of spiral arms or active star-forming regions are discernible. There is no clear evidence of any major interactions or mergers, with a fairly undisturbed appearance.
