The observed galaxy presents as a relatively small, disk-shaped structure. It displays a bright, concentrated central bulge indicative of a high stellar density in this region. The disk appears somewhat inclined to our line of sight, suggesting a possible spiral structure, though the arms are not clearly defined. A slight warp or asymmetry is present in the outer regions of the disk. The galaxy exhibits a range of colors, with the central bulge appearing more yellow-white, implying an older stellar population. The outer regions of the disk show a bluer hue, potentially indicating the presence of younger, hotter stars and ongoing star formation. There is evidence of some dust lanes or obscuration within the disk, particularly near the central bulge. Faint tidal features are visible in close proximity to the galaxy. Overall, this galaxy exhibits features suggesting both an aging stellar population and ongoing star formation, possibly accompanied by interactions with other galaxies.
