The galaxy presents as a slightly elongated, moderately luminous object with a smooth overall structure. It exhibits a dominant central bulge that appears yellowish-orange, suggesting a population of older stars. There is a fainter, diffuse bluish component extending from the bulge, potentially indicating some ongoing star formation within a disk-like structure. The galaxy does not display any obvious spiral arm structure or significant dust lanes in this imaging. It seems relatively undisturbed, showing no major signs of a recent or ongoing merger event, though there is some slight irregularity in its shape. Overall, it appears to be an intermediate mass galaxy with a significant spheroidal component.
