The galaxy presents as a centrally concentrated, relatively smooth structure with an elliptical morphology. The core exhibits a bright, concentrated luminosity, indicating a possible active galactic nucleus or a dense stellar population. The isophotes appear to be elongated but not highly flattened, suggesting an E4-E5 classification on the Hubble scale. The galaxy's color is generally redder overall, indicative of an older stellar population with lower levels of ongoing star formation. There may be very faint indications of a slight warp or tidal feature, but without higher resolution imaging, this cannot be confirmed. Overall, it appears to be a well-formed, relatively undisturbed early-type galaxy.
