The galaxy presents as an elliptical or lenticular type, with a smooth, concentrated morphology. It is characterized by a noticeable lack of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a yellowish-orange hue, possibly indicative of an older stellar population and relatively low star formation activity. There appears to be another galaxy interacting with this galaxy, as there are two separate bodies that seem to be merging together. The galaxy appears to be moderately elongated, departing somewhat from a perfectly circular shape. There also seems to be a relatively round halo surrounding this galaxy, though it is difficult to see clearly.
