The galaxy presents a disturbed morphology, potentially indicative of a merger or interaction. There is no clearly defined spiral structure. The central region exhibits a concentrated, brighter luminosity, suggesting a relatively active galactic nucleus or a dense stellar population. The overall color appears somewhat blue, implying the presence of younger, hotter stars and ongoing star formation activity. Faint tidal tails or bridges are suspected, further supporting the hypothesis of an interaction. The galaxy appears relatively compact in size.
