The galaxy presents as a relatively smooth, but not perfectly circular, structure. There is a slight elongation suggesting a deviation from a perfect elliptical shape. The galaxy appears to be centrally concentrated, with the light intensity decreasing gradually from the center outwards. There are suggestions of minor internal disturbances, possibly indicating ongoing or recent interactions, but no major merger events are readily apparent. Color variation is visible, with a generally redder hue toward the central region, potentially indicating an older stellar population, while bluer regions appear scattered throughout the disk. The overall morphology suggests an intermediate stage of galaxy evolution.
