This galaxy presents a relatively smooth appearance, suggesting a lack of prominent spiral arms or a well-defined disk structure. It exhibits a somewhat elongated, intermediate shape between round and cigar-shaped. The central region displays a brighter concentration of light, indicative of a galactic bulge, though it does not appear exceptionally pronounced. There is some visual evidence of disturbances or asymmetries in the outer regions, possibly hinting at minor gravitational interactions or past merger events. Overall, the galaxy's morphology leans towards a more elliptical or lenticular classification, possibly with ongoing or recent minor interactions affecting its structure. The dominant blueish color suggests active star formation, with a possible presence of younger, hotter stars.
