The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. The light profile appears centrally concentrated. The galaxy exhibits a blue hue, particularly within the central region. There are no distinct spiral arms or bar structures visible. The overall shape is somewhat rounded. There is a faint indication of asymmetry or minor disturbances in the outer regions, possibly indicating past interactions. The observed color implies ongoing star formation, although potentially at a moderate to low rate. The galaxy does not obviously show any signs of a major merger.