The galaxy presents an elongated morphology, possibly indicative of a disk-like structure viewed at an angle. Its overall color appears yellowish-red, suggesting a population of older stars and a relatively low rate of ongoing star formation, with the light likely dominated by redder wavelengths. Two brighter, somewhat diffuse regions are visible, which could represent concentrations of stars or active galactic nuclei. The presence of fainter, diffuse material extending from the central region hints at possible tidal interactions or past merger events. The galaxy's overall structure appears to be disturbed, potentially indicating a system undergoing or recovering from a gravitational interaction. There is evidence of asymmetry in the distribution of light, with one side appearing more extended than the other.
