The galaxy exhibits a primarily smooth morphology, with an apparent lack of distinct spiral arms or a prominent galactic disk. It presents an elliptical shape, with a moderate degree of elongation. A color gradient is observed across the galaxy, transitioning from a reddish hue at one end to a bluer tint at the opposite end. The color variation suggests a possible difference in stellar populations across the galaxy, with older, redder stars potentially concentrated in one region and younger, bluer stars in another. Based on the overall structure, the galaxy could be undergoing a minor merger. A small, compact object is connected to the end of the galaxy exhibiting the reddish hue. This suggests the possibility that the galaxy may be interacting with and tidally disrupting a dwarf galaxy.
