The galaxy presents a largely smooth, rounded morphology, with minimal discernible internal structure. The light distribution appears centrally concentrated, suggesting a dominant spheroidal component. The galaxy exhibits a color gradient, appearing relatively redder towards the center and slightly bluer in the outer regions. There are no obvious spiral arms or a prominent disk structure visible in the image, supporting a classification as an elliptical or lenticular galaxy. Faint irregularities are present, but appear to not disrupt the general structure of the galaxy. There is no apparent merger with another galaxy, nor any significant tidal disturbance.
