The galaxy appears as a centrally concentrated object with a relatively compact morphology. It exhibits a dominant smooth, bright core that likely represents a bulge component. Based on its color profile across the g, r, and z bands, there appears to be a color gradient; the central region appears bluer, indicative of younger stellar populations or ongoing star formation. There appears to be evidence of some tidal disturbances as seen in the faint and diffuse light surrounding the central bulge. This suggests that the galaxy may have undergone a minor merger event. The overall morphology does not show a clear spiral arm structure, but the galaxy is not perfectly smooth. This object may be an elliptical galaxy undergoing some disturbance.
