The galaxy presents a largely smooth morphology, appearing elliptical in shape rather than displaying prominent spiral arms or a distinct disk structure. The central region exhibits a high concentration of light, suggesting the presence of a substantial galactic nucleus or bulge.

There is a subtle, almost imperceptible, flattening of the galaxy's overall shape; it's not perfectly spherical, but rather slightly elongated. The color appears generally yellowish-orange, indicative of an older stellar population with less active star formation. There is little evidence of dust lanes or other features commonly associated with ongoing star formation. I note a very slight asymmetry in the distribution of light within the galaxy, though it's difficult to definitively classify it as a disturbance.
