The galaxy presents as a disk-like structure, viewed at an oblique angle. A prominent bulge dominates the central region, exhibiting a yellowish-orange hue, which suggests an older stellar population. The disk component appears relatively smooth with faint spiral arms visible in bluer tones near the outer edges. These arms indicate the presence of younger, hotter stars and ongoing star formation, although this activity appears to be at a relatively low rate. The overall structure suggests minimal signs of recent major merging events, although some minor disturbances within the disk could indicate possible past interactions. The galaxy is moderately luminous, and its morphology is intermediate between a pure elliptical and a fully-fledged spiral galaxy.
