This galaxy exhibits a predominantly smooth morphology, with a concentrated central bulge. The overall shape is generally elliptical, showing a slight elongation. There is no clear evidence of spiral arms or a prominent disk structure. The color gradient suggests a relatively old stellar population, indicated by the reddish-yellow hue concentrated within the central regions. The outer regions appear slightly bluer, implying the presence of some younger stars, though to a lesser extent than in typical spiral galaxies. There is a faint, fuzzy halo surrounding the main body of the galaxy, potentially indicative of a low level of ongoing star formation or the remnants of previous mergers. Overall, the galaxy appears to be relatively undisturbed, lacking significant tidal features or signs of major mergers.
