The galaxy presents a morphology characterized by a prominent central bulge, suggestive of an elliptical or lenticular type. The bulge exhibits a concentrated, bright luminosity with a yellowish hue, potentially indicating an older stellar population. A flattened disk surrounds the bulge, displaying a smoother texture than what would be expected in a spiral galaxy with active star formation. Some irregular light distribution can be observed with some faint blue patches, likely indicating some on-going star formation, however minimal. The galaxy does not display any obvious signs of a major merger or significant tidal disturbance. The overall shape appears more elliptical, with the axial ratio slightly elongated. The galaxy appears relatively isolated.
