The galaxy presents a largely smooth morphology, with a notable absence of strong spiral arm structures. It appears elliptical, though not perfectly spherical, tending towards an intermediate shape. The central bulge is prominent and exhibits a yellow-orange hue, suggestive of an older stellar population. There is some evidence of a disk component, though it is not sharply defined. The galaxy shows no signs of ongoing major mergers, though a minor disturbance might be present. Star formation activity is low, contributing to the redder color indices.
