The galaxy exhibits a moderately bright central region with a concentrated core. The primary body of the galaxy appears somewhat amorphous, lacking a clearly defined spiral or elliptical structure. There is evidence of a faint, extended halo or disk surrounding the central region, possibly composed of stellar material or gas. The overall color profile suggests a mix of stellar populations, with a relatively brighter blue hue in the central region, potentially indicating recent star formation, surrounded by a greenish halo. There appears to be some distortion or irregularity in the galaxy's outer regions, suggesting a possible ongoing or past interaction or disturbance. The observed light distribution is somewhat clumpy and diffuse, which may indicate complex internal dynamics or the presence of dust obscuration.
