The galaxy presents as a somewhat diffuse, elliptical-like structure, appearing more elongated than perfectly spherical. It exhibits a central bulge with a high concentration of yellow-white light, suggestive of an older stellar population and lower rates of star formation. A very faint disk-like structure may be present. There is a slight asymmetry in its overall shape, possibly indicating a minor gravitational disturbance or interaction with another nearby galaxy in the past. Faint redder regions are visible, which could be areas of dust obscuration or localized regions of more recent star formation. The system lacks prominent spiral arms or strong evidence of ongoing major star formation. Overall, it appears to be a relatively evolved system with an estimated stellar mass near the higher end of the mass function.
