This galaxy presents a morphology consistent with a barred spiral. It exhibits a central bulge that appears smooth and concentrated, with an elongated shape indicative of a significant bar structure. The galaxy's disk component seems relatively faint and contains a small number of visible distinct spiral arms. The overall color profile suggests a mixture of stellar populations with a relatively high amount of older stars. The color of the central bulge is more yellow than the outer areas of the galaxy, which could be due to the increased abundance of older, cooler stars. The galaxy appears to be undergoing a minor gravitational interaction, with a likely dwarf galaxy, though this could be a background object.
