The galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a yellowish hue, which may indicate an older stellar population or a significant dust presence. There is a subtle gradient of color as one moves outward from the center. The outer regions appear slightly bluer, hinting at the presence of younger, hotter stars. The galaxy is neither perfectly spherical nor highly elongated, appearing somewhere in between. There is no obvious sign of a prominent disk structure or spiral arms. There do not appear to be any major disturbances or tidal features indicative of a recent major merger.
