The galaxy presents as a disturbed system. There is evidence of a disk, however it is not clearly defined. The overall structure appears irregular, suggestive of possible tidal interactions or a recent merger event. One distinct component is an elongated arm or tail-like feature exhibiting a yellowish-orange hue, possibly indicating older stellar populations within this structure. Another region towards the center is more condensed and exhibits a more uniform color. This central region is likely the main body of the galaxy, or one of the main progenitor galaxies. It appears slightly elongated. The tidal tail feature is separate from this central region, possibly indicating that it is an ongoing interaction, and that it is not an evolved system. Overall, the galaxy shows characteristics of a mid-mass, actively star-forming galaxy experiencing some form of gravitational disturbance.
