The galaxy presents as a smooth, elliptical form with a high degree of central concentration. The light profile appears consistent with a single Sérsic component with a n value less than 1, suggesting a disk-like structure with an absence of prominent spiral arms or a bulge.  The color gradient is subtle, with the central region appearing slightly bluer than the outer regions. There is a moderate inclination relative to our line of sight, evidenced by the elongated shape. Based on its morphology, it is possibly undergoing minor interactions. The galaxy exhibits a relatively low star formation rate. The neutral hydrogen content is within reasonable bounds.
