The galaxy presents as an extended, cigar-shaped morphology. There is evidence of tidal features or a minor interaction, with a noticeable extension or plume emanating from one end. This plume exhibits a bluer color, suggestive of ongoing star formation. The primary body of the galaxy shows a smoother, more concentrated light distribution, with a redder hue indicative of an older stellar population. Overall, the galaxy is likely in a transitional state, possibly experiencing or recovering from a merger event.
