The galaxy presents as a system likely undergoing an interaction or merger. Two distinct luminous components are observed. The larger of the two components exhibits a slightly elongated, non-circular shape. It is brighter and yellowish, potentially indicative of an older stellar population. The second, smaller component is more rounded and slightly redder. It is fainter than the larger object. There is some evidence of tidal features or faint light connecting the two components, which is suggestive of gravitational interaction. There is no distinct spiral arm structure or prominent dust lanes visible in either component. Overall, the system appears relatively smooth, suggesting that, if this is a merger, it may be in a mid- to late-stage of the process.
