The galaxy presents an elliptical morphology, appearing largely smooth in structure with a concentrated central region. The light distribution is relatively symmetric. Color gradients are subtle, with a yellowish hue dominating the core, transitioning to slightly bluer tones in the outer regions. The overall appearance suggests a mature stellar population. No prominent spiral arms or distinct dust lanes are discernible. There is no indication of a major ongoing merger event, though minor asymmetries or disturbances cannot be ruled out. The galaxy is moderately luminous. The estimated size corresponds to a galaxy with a mass comparable to the Milky Way, however it is difficult to discern an exact size from the image alone. Star formation is subdued.
