The galaxy presents as a relatively smooth, elliptical-like structure. It is elongated in shape, approximately twice as long as it is wide, resembling a cigar. A bright, concentrated central bulge is visible, which gradually diffuses into the surrounding halo. The galaxy exhibits a blue hue, primarily concentrated in the central regions, which suggests ongoing star formation. The outer regions appear more diffuse and display a slightly redder color, potentially indicative of an older stellar population. There is slight evidence of a possible minor disturbance or interaction, as the outer halo appears slightly asymmetrical on one side. Overall, the galaxy appears relatively undisturbed with no major morphological disruptions.
