The galaxy presents as an elliptical-like structure with a generally smooth morphology. It exhibits a concentrated central bulge that appears primarily yellow, suggesting a significant population of older stars. The galaxy appears somewhat elongated, tending towards a cigar shape. Faint blue hues are observed in the outer regions, potentially indicative of some ongoing, but limited, star formation. There is no discernible evidence of a major merger event or significant tidal disturbances, but some minor asymmetry or disturbance cannot be ruled out. The galaxy appears relatively isolated in this field.
