The galaxy presents a lenticular, somewhat oblong morphology with a smooth, centralized light distribution. The color profile reveals a galaxy characterized by a significant population of older stars, as evidenced by the redder hues. There is a faint blue tint, indicative of a small amount of more recent star formation. No distinct spiral arms or a prominent central bar structure are visible. There is a faint indication of disturbances in the shape, suggestive of tidal interactions or a minor merger event in its past.
