The galaxy exhibits a prominent central bulge region, displaying a yellowish-white color gradient indicative of an older stellar population. Surrounding the bulge, a fainter, more diffuse disk is visible, oriented roughly face-on. This disk shows subtle hints of spiral arm structure, with flocculent and patchy regions of bluer light suggesting ongoing star formation. The spiral arms are not tightly wound but rather open and somewhat fragmented. The overall structure of the galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The galaxy appears to have a moderate to large-sized bulge relative to its disk. There is a subtle bar-like structure that runs through the central region. Dust lanes are not clearly discernible, however, there may be obscuration near the bar and regions of star formation. Overall, this is a spiral galaxy with a well-defined bulge and hints of active star formation in its disk.
