The galaxy presents as a singular, somewhat regular, object with a generally elliptical morphology. The light distribution is relatively smooth and centrally concentrated. The overall color profile suggests a redder object, implying an older stellar population and/or significant dust obscuration, which is consistent with a quiescent galaxy that has largely ceased active star formation. No prominent spiral arms, bars, or other disk-like features are clearly discernible. There are no signs of any major tidal disturbances or ongoing mergers that would significantly distort the galaxy's overall shape. The object appears moderately luminous.
