The galaxy presents a generally smooth morphology, with a highly concentrated central bulge that graduates outward to a less dense halo. The central region exhibits a yellowish hue, possibly indicating an older stellar population with decreased star formation activity. The outer regions appear slightly bluer, suggesting a younger stellar population compared to the central bulge, although active star formation appears to be low overall. The galaxy exhibits a high degree of rotational symmetry, with no obvious signs of major disturbances or ongoing mergers. The shape appears to be somewhere between elliptical and disc-like. The galaxy's overall structure is relatively undisturbed. The estimated size is approximately 4.7 kpc in radius.
