The galaxy presents a smooth, elongated morphology, appearing as a cigar shape. The light profile suggests a relatively high degree of central concentration. The color appears yellowish-white, indicative of an older stellar population with a reduced rate of star formation. The galaxy does not exhibit any readily apparent spiral arm structures or significant dust lanes. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy appears generally undisturbed with a smooth, centralized light distribution.
