The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge, surrounded by a more diffuse halo. There may be some evidence of ongoing or recent interaction with another galaxy, as there are possible disturbances in the outer regions of the halo. The colors appear to be relatively uniform throughout the galaxy, suggesting an older stellar population with minimal ongoing star formation, though a hint of blue tinges in areas may indicate otherwise. The axial ratio indicates a possible elliptical shape that is nearly round. Overall, this appears to be a galaxy with moderate mass that is likely undergoing significant interaction.
