The galaxy presents a generally elliptical morphology, though not perfectly spherical. It appears as a concentrated central bulge surrounded by a fainter, more diffuse halo. The central bulge exhibits a yellowish-white hue, indicative of an older stellar population with lower levels of on-going star formation. The outer regions appear slightly bluer, suggesting the presence of some younger stars, though the overall star formation rate appears relatively low. The overall structure is largely smooth, without the presence of strong spiral arms or significant dust lanes. There is no visual evidence of a major merger, though a possible minor disturbance or interaction can't be ruled out based on slight irregular features. The galaxy is moderately large and luminous.
