This galaxy exhibits a morphology consistent with a potential merger or a galaxy undergoing significant tidal disruption. The light distribution is elongated and somewhat irregular. There are two distinct, bright cores or concentrations of light within the galaxy's body, suggesting either two interacting galaxies or the remnant of a single galaxy with a strongly disturbed nucleus. 

The overall color of the galaxy appears relatively red/yellowish, which may indicate an older stellar population and/or significant dust content. The general shape is neither clearly elliptical nor spiral; it falls somewhere in between, likely due to ongoing interactions that have scrambled its original structure. There's some faint hint of extended material surrounding the main body, potentially tidal tails, but more data would be needed to confirm their presence and extent. The galaxy shows signs of moderate star formation.
