The galaxy presents a largely smooth and elliptical morphology. The light distribution is concentrated toward the center, with a gradual decrease in intensity outwards. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. Fainter, greenish light is observed in the outer regions of the disk. The galaxy does not appear to show evidence of strong spiral arm structures or significant dust lanes. The overall appearance suggests a relatively evolved system, with a likely low star formation rate. No major interactions or disturbances are readily apparent in the image. The galaxy is moderately luminous.