The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, featureless morphology. The luminosity profile appears centrally concentrated, with the light gradually decreasing towards the outer regions. The galaxy exhibits a slight elongation, with a suggestion of being "in between" round and cigar-shaped. There are no visually apparent signs of spiral arms or a prominent disk structure. There is no visible ongoing major merger or significant tidal disturbance. Faint traces of potential minor disturbances might be present, but this needs further investigation with higher resolution data. The galaxy's color is somewhat yellowish-white, suggesting a relatively older stellar population, with ongoing but low star formation. 
