The galaxy presents as a moderately bright, elliptical-shaped structure with a smooth, diffuse light distribution. It appears predominantly featureless, with no readily discernible spiral arms or bar structures. The central region exhibits a slightly higher concentration of light, indicating the presence of a galactic nucleus. There is a subtle color gradient, trending towards redder hues in the central region and slightly bluer towards the outer edges. There are no visible signs of active star formation regions or dust lanes within the galaxy. The galaxy appears relatively isolated, without any clear evidence of ongoing or recent major merger events. However, there is some subtle, localized disturbance in its morphology, suggesting possible minor interactions or internal dynamic processes.
