This galaxy exhibits a disturbed morphology, strongly suggestive of an ongoing or recent merger event. The primary body of the galaxy appears somewhat smooth, but shows clear evidence of tidal interactions. There are two particularly bright, concentrated regions within the galaxy's central area, possibly representing the nuclei of the merging galaxies. The overall shape deviates significantly from a regular elliptical or spiral form, presenting a somewhat irregular profile. The color profile suggests a mixed stellar population. The presence of reddish hues indicates older stars, while the contribution of bluer colors, especially in the central regions, suggests recent or ongoing star formation. The estimated luminosity of the galaxy is high, potentially linked to increased star formation activity triggered by the merger. The interaction appears to be a major disturbance, disrupting the original structure significantly. 
