The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. The primary body of the galaxy appears elongated and somewhat irregular. There is evidence of tidal features or debris extending from the main body, further indicating gravitational interaction. The color of the galaxy leans towards the redder end of the spectrum, implying a population of older stars and potentially a reduced rate of star formation compared to bluer galaxies. There may be some dust obscuration affecting the light emitted. A distinct, compact source is visible in proximity to the galaxy. Overall, the galaxy's appearance suggests a complex evolutionary history influenced by interactions with other galaxies.
