The galaxy presents a largely smooth and rounded morphology, with no readily discernible spiral arms or bar structures visible. The galaxy's core exhibits a bright, concentrated luminosity suggesting a significant stellar population or active galactic nucleus. The overall color profile appears to be moderately red, implying an older stellar population. A slight deviation in circularity is observed, possibly indicative of a minor interaction or past merger event. The galaxy is relatively compact, with an estimated half-light radius of approximately 3.5 kiloparsecs. There is a small amount of blue light, suggesting some ongoing star formation. Overall, the galaxy appears to be a relatively massive elliptical galaxy.
