The galaxy exhibits an irregular morphology, suggesting it is undergoing a dynamic interaction or merger. The light distribution reveals two distinct components, one with a yellowish hue and the other with a reddish hue. These components are offset and appear connected, possibly indicative of tidal effects or ongoing galactic cannibalism. The yellowish component is more diffuse, potentially containing older stellar populations or dust obscuration. The reddish component appears more compact and may contain regions of active star formation, given the presence of shorter wavelengths. Overall, the galaxy does not exhibit grand spiral arms or a well-defined elliptical shape, further suggesting that it is currently undergoing a morphological transformation due to some form of gravitational disturbance. The galaxy is relatively small, and has low to moderate star formation activity.