The galaxy presents a somewhat disturbed morphology, displaying features suggestive of an ongoing or recent interaction. The central region exhibits a concentrated, yellowish glow, possibly indicating an older stellar population and reduced star formation activity in the core.

Surrounding the central region, faint, diffuse bluish-green extensions are visible. These may represent regions of more recent star formation, possibly triggered by the interaction that is disrupting its overall structure. The galaxy's shape is elongated, deviating significantly from a circular morphology. This cigar-like shape, along with the hints of disturbance, supports the hypothesis of an ongoing or recent merger event. There is also a hint of a tidal tail or arm extending from one side, further suggesting the galaxy is in an interactive state.
