The galaxy presents a flattened, elongated morphology, suggesting an elliptical classification. The color profile indicates a concentration of older stellar populations, primarily in the redder bands. The object exhibits a smooth, largely featureless appearance. A slight distortion is visible at the edges of the galaxy but may not be significant. There is no indication of ongoing star formation, which aligns with the observed color profile. No signs of mergers or tidal tails are observed. The galaxy appears to be relatively undisturbed.
