The galaxy presents as a flattened, elliptical morphology. A bright, condensed central bulge dominates the core region, exhibiting a yellowish-white hue. This central concentration gradually diffuses into a less luminous, somewhat bluer disk. The disk appears relatively smooth, with no obvious spiral arm structures visible. The galaxy's overall color suggests a population of older stars, particularly in the bulge. There is a slight elongation to the galaxy, appearing cigar-shaped. No signs of significant recent merger activity are apparent, although a faint distortion or minor disturbance cannot be entirely ruled out. The galaxy exhibits a low rate of star formation.