The galaxy presents as a somewhat elongated, disk-like structure with a moderately bright central bulge. The color gradient suggests potential variations in stellar populations, with a reddish hue concentrated toward the galactic center, possibly indicating older stars or increased dust obscuration. The outer regions of the galaxy appear bluer, suggesting the presence of younger, hotter stars, and ongoing star formation. There are faint indications of spiral arm structures, although they appear somewhat disrupted or ill-defined, hinting at possible past interactions or internal disturbances. The overall morphology appears to fall somewhere between a smooth elliptical galaxy and a well-defined spiral, suggesting it is a transition type. The light distribution indicates a concentration of mass towards the center, typical of most galaxies.
