The galaxy exhibits a morphology suggestive of an interacting system, with noticeable disturbances in its overall structure. The main body of the galaxy appears relatively smooth but with some evidence of an asymmetric bulge. A distinct plume of stellar material extends outwards, exhibiting a gradient in color, transitioning from a bluer hue near the central region to a more yellow-orange tint further away. This plume might be indicative of tidal forces stripping material from the galaxy or a recent burst of star formation along its length. The galaxy's faint outer regions appear diffuse and irregular, further supporting the hypothesis of a merging event or significant gravitational interaction with another object. The overall color index suggests the presence of both older stellar populations and recent star formation activity.
