The galaxy presents as an elliptical morphology, appearing generally smooth and well-defined. There is a concentrated central bulge exhibiting a yellowish hue, potentially indicating an older stellar population and/or dust obscuration. The overall shape is relatively round. Although generally smooth in appearance, a subtle asymmetry is observed, hinting at a possible minor gravitational interaction or internal disturbance. The galaxy appears to be relatively quiescent, with a low rate of star formation. Its color suggests a spectral energy distribution that is redder than that of actively star-forming galaxies. Based on the size and color, this galaxy is likely quite massive.
