The galaxy presents as a slightly elongated, lenticular-like structure. It exhibits a smooth, centrally concentrated light distribution, suggesting a dominant bulge component with a more diffuse disk. The color gradient is subtle, transitioning from a yellowish core to a slightly bluer, fainter outer region. This color gradient suggests a higher concentration of older stars in the central bulge and a younger stellar population in the surrounding disk. There is no clear evidence of spiral arm structures or prominent dust lanes. The galaxy does not appear to be undergoing a major merger, although very minor disturbances cannot be ruled out.
