The galaxy presents as a primarily smooth object, exhibiting a relatively round morphology. There is a subtle suggestion of a disk structure; however, the dominant characteristic is its smoothness. A minor irregularity is visible, but it could be the result of noise or the remnants of a small tidal disruption. The galaxy presents a color profile consistent with an older stellar population, with a high fraction of light emitted in the redder bands. This is indicative of fewer young, blue stars and a greater population of red giants. The object shows no indication of a major merger or active galactic nucleus in the wavelengths captured.
