The galaxy presents a largely smooth morphology, with a dominant central bulge. The light distribution appears relatively uniform, lacking any prominent spiral arm structures or significant dust lane features. The shape approximates a circular form, with an absence of strong ellipticity. A slight color gradient is visible, with the central region appearing more yellow-gold in comparison to the outer regions of the galactic halo. This may indicate an older stellar population concentrated towards the core. There is a subtle suggestion of possible minor disturbances in the outer halo, but nothing that would definitively suggest an active merging event. Overall, the galaxy's appearance is consistent with that of an early-type galaxy, likely an elliptical or lenticular system.
