The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright core which gradually diffuses outward. The overall color is a yellowish-white, suggesting an older stellar population with lower levels of ongoing star formation. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears undisturbed, showing no signs of major mergers or tidal interactions. The roundness indicates a possible E0-E2 classification on the Hubble sequence.
