The galaxy presents with a disturbed morphology, suggestive of an ongoing or recent interaction. The central region exhibits a concentrated luminosity, possibly indicative of an older stellar population or an active galactic nucleus, appearing as a yellowish-orange hue. Extending from the central region is a distinct arm or tidal feature with a redder color. This could be indicative of a region with increased dust content or ongoing star formation. There is some evidence of diffuse blue light towards the disk of the galaxy, suggesting the presence of younger, hotter stars and, thus, star-forming regions. Overall, the galaxy appears to be of intermediate size and mass with relatively active star formation. The system displays signs of gravitational disturbance. A significant portion of the light is more concentrated than would be expected in a purely spiral morphology.
