The galaxy presents a generally elliptical morphology, appearing largely smooth and without prominent spiral arm structures. The central region exhibits a high concentration of luminosity, indicative of a significant stellar population or active galactic nucleus. The galaxy displays a color gradient, transitioning from a yellowish core to slightly redder outer regions. There is a faint suggestion of a tidal tail or minor disturbance extending from one side, which may indicate a past or ongoing interaction with another galaxy, or an internal dynamic process. The shape is not perfectly circular; it appears elongated.
