This galaxy presents a somewhat disturbed morphology. The primary structure suggests a disk-like system, though without clearly defined spiral arms. There's a noticeable central bulge that appears bright and concentrated, transitioning outwards to a less defined, more diffuse disk component. The color profile indicates a mix of stellar populations. The central bulge appears more yellow/orange, suggesting older, redder stars. The outer regions exhibit a bluer hue, potentially indicating the presence of younger, hotter stars and ongoing star formation, although at relatively low levels. There's a secondary object nearby that could potentially be a dwarf galaxy. The general shape of the disk is somewhat irregular, possibly a result of gravitational interactions or past mergers.
