The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright, yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a slightly bluer tint, possibly indicating the presence of a younger stellar population or ongoing star formation within the galactic disk. The galaxy's shape is neither perfectly spherical nor highly elongated, appearing somewhat intermediate. There are no readily apparent signs of major disturbances or ongoing mergers, although subtle asymmetries could be present. Faint extensions of the galactic disc may be present.
