The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, elliptical morphology. The central region shows a concentration of light, likely the galactic bulge, which displays a yellowish hue. Extending outwards, a faint disk is visible, with hints of spiral arms. The disk component appears bluer in color compared to the central bulge, suggestive of younger stellar populations or ongoing star formation. There is no visible evidence of active galactic nuclei or prominent dust lanes. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions with nearby galaxies.
