The galaxy presents as a centrally concentrated, relatively smooth object. Its overall form appears elliptical or lenticular, displaying a high degree of radial symmetry. There's a pronounced central bulge, exhibiting a yellow hue. The color gradient suggests a stellar population dominated by older, redder stars within the bulge. The outer regions of the galaxy transition to a bluer color profile, hinting at the presence of younger, bluer stars, and possibly some ongoing star formation, although the rate seems to be low. There is no discernible disk structure or spiral arm morphology. No significant tidal features or evidence of recent major mergers are apparent. There may be some faint disturbances, indicating minor gravitational interactions or minor mergers. The galaxy's shape is mostly round, as opposed to elongated, but the roundness may be an artifact of its distance. 
