The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, appearing bright and slightly yellow-tinted, suggestive of an older stellar population. Progressing outward from the core, the galaxy displays a gradual decrease in surface brightness. A subtle flattening is observed; the galaxy is not perfectly spherical but tends toward an intermediate ellipticity. There is a hint of disk-like structure present, but this galaxy does not display prominent spiral arms or significant irregular features. There is no strong evidence of ongoing merger activity or major tidal disturbances. The overall appearance is consistent with a galaxy that is not currently undergoing intense star formation, with minimal indication of dust lanes or regions of intense HII emission.
