The galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merger. A dominant, somewhat diffuse, component displays a central concentration, indicative of a possible spheroidal structure. This component appears relatively smooth, suggesting an older stellar population.

Adjacent to this is a distinct, more compact and luminous region, offset from the center of the main body. This secondary component appears more yellow/orange in color, suggesting the presence of a population of older stars or significant dust obscuration.

There is visible tidal stream extending away from this brighter, yellowish object, suggesting that the two components are merging. The overall form is disturbed, with the suggestion of tidal tails or distorted spiral arms. The galaxy appears to be actively undergoing some type of dynamical process, either an advanced state of merger or a strong interaction with another galaxy.
