This galaxy exhibits a morphology consistent with a spiral galaxy, likely seen at an angle. The central bulge appears bright and yellowish, suggesting a population of older stars. Surrounding the bulge, we observe a fainter, bluish disk, possibly indicative of ongoing star formation. Some slight disturbances are observed, and it is not clear if these disturbances are from interactions with another galaxy or another mechanism. Given the color distribution, the galaxy likely possesses a moderate stellar mass and star formation rate.
