The galaxy presents as a relatively smooth, elliptical morphology. The central region appears to be composed of older stellar populations, as evidenced by the yellowish-white hue. Surrounding the central region, a slightly bluer disk-like structure is observable, suggesting the presence of some ongoing or recent star formation. The galaxy's overall shape is somewhat elongated, deviating from a perfect sphere, potentially indicating a moderate amount of rotational support or a past minor merger event. No prominent spiral arms, bars, or other significant structural features are discernible. The galaxy appears relatively isolated, with no obvious signs of major interactions with neighboring galaxies or tidal disturbances.
