This galaxy appears to be a disk galaxy, viewed at a slight angle. It exhibits a relatively smooth, centrally concentrated light distribution, with some evidence of a slightly brighter, more compact core region. There are hints of spiral arm structure but they are indistinct. The overall color suggests a mix of stellar populations, with perhaps slightly bluer regions in the central area, potentially indicative of ongoing star formation. There are some irregularities in the outer regions, possibly due to minor interactions or disturbances. There appears to be minimal evidence of a major merger event; the galaxy does not seem to be heavily disrupted.
