The galaxy presents a somewhat elliptical morphology, showing a smooth, centralized bulge. There is a subtle indication of a disk structure. The color profile indicates an older stellar population, dominated by redder hues in the central region. Fainter, bluer light extends outwards, suggesting possible areas of recent, yet minimal, star formation. Faint tidal tails are visible, indicating possible merger activity. The galaxy appears to be undergoing gravitational disturbance with evidence suggesting an interaction with another galaxy.
