The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated core. Its overall form is elongated, with the major axis extending roughly east-west. The color gradient transitions smoothly from a yellowish-white at the nucleus to a bluish hue in the outer regions. There is a notable absence of distinct spiral arms or well-defined dust lanes. The galaxy shows a mild degree of asymmetry, with some subtle disturbances in the outer regions. These may be related to a minor interaction with another galaxy or the recent accretion of smaller objects. Star formation seems to be low within the galaxy, with some regions of slightly higher activity in the periphery.
