The galaxy presents a primarily smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or significant dust lanes. The light distribution is concentrated towards the center, indicating a prominent bulge. The galaxy exhibits a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation. The overall shape is close to round, though a slight elongation may be present. There is no clear evidence of any recent or ongoing major merger activity. There are also some areas of red, which indicates areas of more dust or nebulae, but these appear faint.
