The galaxy appears to be a spiral type, but observed at an angle that makes the spiral arms difficult to discern. It presents a somewhat amorphous structure. The galaxy exhibits a prominent central bulge, bright and concentrated, suggesting a higher density of stars in that region. The color profile indicates a likely evolved stellar population; the yellowish-red hue suggests older stars dominate the light output. There is a hint of bluer regions in the outer reaches of the galaxy, possibly indicating pockets of ongoing, albeit relatively low, star formation. Overall, the galaxy appears relatively undisturbed, with no major signs of recent mergers or tidal interactions, although there are some asymmetries in the outer disk that indicate possible minor interaction or disturbance.
