The galaxy presents as a generally smooth, elliptical structure with a highly elongated shape. The core exhibits a bright, concentrated luminosity, which transitions into a fainter, more diffuse halo. There are no prominent spiral arms, bars, or distinct dust lanes visible.

Color gradients are subtle but present, with a bluer hue towards the central region, suggesting potential ongoing, but subdued, star formation. The outer regions appear redder, indicating a population of older stars. There are no obvious signs of interaction or major disturbances. The galaxy does not appear to be undergoing an active merging event, but minor tidal features cannot be ruled out.
