The galaxy presents as an elliptical morphology with a smooth, centralized luminosity profile. The core exhibits a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a slightly redder tone, indicating the presence of evolved stars within the galaxy's halo. No discernible spiral arms, dust lanes, or active star-forming regions are visible. The overall shape appears relatively round. There's no apparent tidal disturbance or merger activity influencing the structure.
