The galaxy presents as a centrally concentrated object, likely elliptical or lenticular in morphology. It exhibits a smooth light distribution with minimal discernible structure or spiral arms. The color profile suggests an older stellar population, with a yellowish hue indicating a dominance of evolved stars and reduced ongoing star formation. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or mergers. There are hints of a slightly elongated shape, deviating from perfect circularity. The galaxy appears generally quiescent.
