The galaxy presents as a somewhat elongated, elliptical object with a smooth, diffuse light distribution. The central region exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars towards the core. The overall color appears to be slightly blue-white, indicating a population of younger, hotter stars, though the smoothness of the light suggests that the star formation may not be extremely active. There appears to be some disturbance to the galaxy's structure, perhaps it is undergoing a minor merger or tidal interaction. The shape is not perfectly spherical, displaying a more cigar-like or elongated morphology. There is no clear indication of spiral arms or a prominent disk.
