The galaxy presents as a relatively compact, elliptical-like structure, exhibiting a smooth light distribution. There are no clear spiral arms or bar features visible. The light profile suggests a dominant, centrally concentrated bulge. There is some subtle evidence of a slight tidal disturbance, possibly indicating a past minor merger event. The overall color is yellowish-orange, suggesting an older stellar population with lower rates of ongoing star formation. The galaxy appears mostly undisturbed, likely relaxed and approaching quiescence.