The galaxy presents as a relatively smooth, rounded object. It exhibits a slight elongation, appearing more "in between" than perfectly circular, but does not deviate significantly from a circular shape. The galaxy displays a prominent central bulge that transitions smoothly into the outer regions, showing no distinct spiral arm structure in the available imaging. There is no indication of recent or ongoing major merger activity, although subtle signs of a minor disturbance within the galaxy cannot be entirely ruled out. Color variations are present, with the central bulge showing a yellow hue, suggesting an older stellar population, while the outer regions exhibit bluer tones, which may indicate younger stars or regions of active star formation, albeit at a relatively low rate. Overall, the galaxy appears to be an evolved system, showing signs of both old and more recent stellar populations.
