The observed galaxy exhibits a complex morphology suggestive of an ongoing merger event. The primary structure appears to be a distorted disk galaxy, with an apparent tidal tail extending outwards, indicating gravitational interaction. The color profile displays a strong central concentration of blue light, possibly indicative of recent star formation activity in the core region. This is further supported by the overall irregular shape, which departs significantly from a smooth elliptical or spiral form. There are indications of dust lanes present, although the image resolution limits detailed characterization. Redder hues are visible along the periphery of the disk, hinting at an older stellar population. The object appears relatively compact. Further spectroscopic analysis would be beneficial to confirm the star formation rate and gas metallicity.
