The galaxy presents as an elliptical morphology, with a smooth, spheroidal structure. The central region exhibits a concentrated, bright core indicative of a significant stellar population. There is an orange-yellowish hue, with a decrease in surface brightness as it extends outwards. While largely smooth, subtle irregularities are present, there are no clear spiral arms or prominent dust lanes. The overall shape is nearly circular, but with some variation in its outermost regions. There appears to be evidence of low-level star formation within the galaxy. There are no signs of a major merger event in the image, although some minor disturbances may be present.
