The galaxy presents as a centrally concentrated object, likely an elliptical or lenticular type. The light profile appears smooth and gradually decreases in intensity outwards from the central region. The core is luminous with a yellow-orange hue, suggestive of an older stellar population. The overall shape is elongated and somewhat cigar-shaped, indicating it is not perfectly spherical. There is a faint disk or arm feature that can be perceived within the galaxy. There appear to be minimal signs of recent or ongoing major merger activity, such as tidal tails or strong asymmetries, suggesting the galaxy is relatively undisturbed. The color suggests low current star formation.
