The galaxy appears to be a spiral galaxy with a prominent central bulge. The bulge exhibits a bright, relatively uniform yellowish-white color, suggesting a population of older stars. Surrounding the bulge, a faint disk structure is visible, displaying evidence of spiral arms. These arms show a bluer hue, likely due to the presence of younger, hotter stars and ongoing star formation. The arms seem somewhat loosely wound and patchy, indicating possible disturbances or interactions. There are some redder regions scattered within the disk, these may be areas of dust obscuring the light or HII regions caused by recent star formation. The overall morphology suggests that this galaxy is a later-type spiral, exhibiting a less tightly wound structure than earlier-type spirals. The galaxy does not seem to show any major signs of mergers or tidal disruptions, but some minor disturbances in the disk cannot be ruled out.
