The galaxy appears to be undergoing a significant interaction or merger event. Visually, multiple distinct clumps of luminous material are present, suggesting either multiple galactic nuclei or regions of intense star formation triggered by tidal forces. The overall morphology is highly disturbed, deviating significantly from a regular elliptical or spiral structure. There is a clear dominance of yellow and orange hues within the galaxy, suggesting an older stellar population and/or significant dust obscuration. The lack of strong blue emission hints at a low rate of on-going star formation. The galaxy's shape can best be described as in between an elliptical or a cigar shape, as the galaxy is not spherical but is not strongly elongated. There is clear evidence of tidal tails or bridges extending from the main body of the galaxy, indicative of strong gravitational interactions. The overall profile appears diffuse, lacking a well-defined central bulge or disk. The spatial extent suggests this is a fairly large and massive galaxy.
