The galaxy presents as a relatively smooth, concentrated structure with a slight elongation. The color gradient suggests a more active star forming region within the central bulge, indicated by the yellowish hue. The galaxy appears to be in a relatively isolated state. The overall morphology is consistent with an early-type galaxy, specifically an elliptical galaxy, with a possible hint of a faint disk. There is no indication of any recent major merger events or significant tidal disturbances.
