The galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. Two distinct luminous regions are observed, indicating at least two interacting galactic components. The brighter of the two regions appears relatively smooth, possibly representing a spheroid or bulge component. The second region appears more irregular and diffuse, possibly indicative of tidal disruption or star formation triggered by the interaction. Overall the galaxy appears to have an irregular morphology. There are some indications of possible tidal tails or bridges, but further data would be needed to properly quantify these features. The system displays color gradients, with the brighter region exhibiting a yellower hue, potentially reflecting an older stellar population, and the fainter region has a bluer tint, suggesting more recent star formation.
