The galaxy presents a relatively compact morphology. There are visible features indicating the presence of potential interactions or disturbances. A dominant, somewhat spheroidal component exhibits a yellowish hue, possibly indicating an older stellar population. Dispersed towards the bottom of the galaxy is a region with bluer tones, suggesting ongoing or recent star formation activity. The galaxy appears to be undergoing or have recently undergone a merger. It lacks a well-defined spiral structure. Overall, the galaxy has a moderate degree of irregularity in its shape.
