The galaxy presents as a relatively smooth, elongated structure, likely an elliptical or lenticular type. A distinct color gradient is visible, transitioning from a yellowish core to bluer outer regions. This color variation suggests potential differences in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars distributed further out. The high degree of smoothness in the light distribution points to a galaxy that has undergone significant dynamical relaxation. There are no apparent spiral arms or other features indicative of ongoing major star formation. The overall morphology indicates that the galaxy may have experienced past merging activity, but it currently appears largely undisturbed.
