The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue, indicating an older stellar population. There is minimal evidence of spiral arms or significant star formation regions within the observable structure. The galaxy appears moderately rounded in shape. There is a slight suggestion of a minor disturbance in its overall morphology but no indication of any major merger events. The outer regions of the galaxy diffuse into the background, suggesting a decline in stellar density with increasing distance from the galactic center. Overall, the galaxy appears to be a quiescent, evolved system.
