The galaxy presents as a system undergoing a merger or significant interaction. It exhibits a complex morphology, with possible tidal features or disrupted spiral arms faintly discernible. There are several bright knots or clumps of light visible within the galaxy, indicating regions of potentially high star formation activity or dense stellar populations. The overall color of the galaxy is yellowish to reddish, suggestive of an older stellar population, although the presence of bluer regions indicates ongoing star formation. The core of the galaxy appears diffuse and the overall shape could be described as irregular, which supports the observation of a system that has been disturbed. Overall, the system shows to be moderately rounded, with no long extension along any particular axis.
