The galaxy presents as a relatively smooth, elliptical-like structure. A distinct central bulge is observed, exhibiting a concentrated, bright yellowish-white luminosity, indicating an older stellar population. This light diffuses outward, transitioning into a less concentrated, fainter halo. The halo appears subtly bluer than the central bulge, potentially suggesting a small degree of more recent star formation at greater galactic radii. No prominent spiral arm structures or dust lanes are readily discernible, further supporting a classification towards the elliptical end of the Hubble sequence. The overall morphology suggests a galaxy undergoing relatively low rates of current star formation and with a significant mass. There are no clear indications of major mergers or significant tidal disturbances in its immediate vicinity, pointing toward a relatively isolated evolutionary path.
