The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular type. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The overall shape is close to round, with only a slight deviation towards an elongated form. A subtle color gradient is visible, with a slightly redder hue in the central bulge compared to the bluer outskirts, possibly indicative of differing stellar populations and star formation histories within the galaxy. There is no evidence of strong tidal features or significant asymmetries, implying a relatively quiescent evolutionary state. However, a subtle disturbance on one side suggests a possible past or ongoing minor interaction.
