The galaxy presents an elongated, somewhat irregular morphology. Its overall color appears bluish, suggesting a population of relatively young, hot stars and ongoing star formation. There is a brighter, concentrated region toward the center of the galaxy which could be the bulge or a nucleus. Faint extensions or tidal features may be present, indicating possible gravitational interactions or past mergers. The galaxy's elongated shape could imply it is either an edge-on spiral galaxy, or an elliptical galaxy. The smoothness of the light profile suggests it is more likely to be an elliptical galaxy.
