The galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merger event. The primary body of the galaxy has a centrally concentrated, luminous core, with an overall smooth appearance. A secondary, distinct component is visible nearby, possibly a smaller galaxy in the process of merging. There appears to be some tidal distortion present, possibly a faint bridge connecting the core and the companion, or a faint tidal tail extending from the system. The color gradient suggests a population of older stars in the center, and some hints of bluer, younger stars possibly triggered by the interaction. The system is compact, with an estimated diameter of approximately 4 kpc. There is no apparent spiral structure.
