This galaxy exhibits a roughly elliptical morphology, appearing mostly smooth in texture with a concentrated central bulge. The core region displays a yellowish hue, indicative of an older stellar population. Fainter, diffuse, blue-ish color emissions surround the central bulge, suggesting the presence of some younger stars or ongoing star formation. There may be faint indications of a disk structure, but it is not well-defined and heavily obscured by the smoothness of the galaxy. Minor disturbances may be present based on asymmetry in the surrounding diffuse light. The galaxy appears to be a substantial object, with an estimated diameter of about 8 kpc and a stellar mass around 10^10 solar masses. Observed light suggests that this galaxy is in a transitional state, as star formation has slowed, approaching a quiescent state.