The galaxy presents a predominantly smooth morphology, with minimal evidence of distinct structural features such as spiral arms or a prominent bar. The light distribution appears centrally concentrated, exhibiting a radial profile that gradually diminishes with increasing distance from the core. The shape of the galaxy is observed to be generally elliptical, though not perfectly spherical, and elongated across one axis. Color gradients are subtle, with the central region exhibiting a yellowish hue and the outer regions showing hints of blue in the outer edges of the galaxy. There is no compelling indication of ongoing major merger activity. Slight disturbances may be present.
