The galaxy appears as a centrally concentrated object with a generally smooth morphology. There's a high degree of radial symmetry, suggesting a classification towards the elliptical end of the Hubble sequence. The color is generally redder, indicative of an older stellar population with limited ongoing star formation. The galaxy exhibits a fairly concentrated light profile. There is a small possible companion visible to the left, but it appears diffuse and may simply be noise. There are no clear signs of tidal disturbances or recent mergers present in the image.
