The galaxy presents as a relatively compact object, approximately elliptical in shape. The central region exhibits a higher surface brightness and a somewhat smoother appearance, suggesting a prominent bulge. There are faint hints of spiral arm structures extending outward from the central region, though they are not well-defined. A subtle color gradient is observed, with the central region appearing slightly more yellow or red, while the outer regions tend towards a bluer hue, possibly indicative of younger stellar populations in the disk. 

There is evidence of possible tidal distortions or interactions. A faint extension or plume can be seen emanating from the galaxy. It's also possible that there is a minor disturbance or a merger event that may be underway, contributing to the asymmetric morphology. However, further observations are needed to confirm this.
