The galaxy exhibits a largely smooth morphology. The central region shows a concentrated bulge, with a somewhat amorphous, extended disk component. Color gradients suggest varying stellar populations, with the central bulge appearing redder, possibly indicating older stars. A blue-ish glow is visible around the galaxy, which may indicate younger stars or ongoing star formation. There's a slight suggestion of asymmetry or a minor disturbance in the overall structure. The galaxy displays a relatively compact appearance, with an estimated physical size of a few kiloparsecs across. The overall visual impression is of a galaxy transitioning between elliptical and spiral classifications.
