The galaxy presents as a gravitationally interacting system, exhibiting characteristics of a merging or disturbed morphology. A central, brighter core of the galaxy displays a yellowish-white hue, potentially indicating an older stellar population. Emanating from this core are diffuse, less luminous structures with a bluer tint, indicative of ongoing or recent star formation. These features suggest a possible spiral or disk-like component undergoing disruption due to tidal forces or gravitational interactions. The overall structure appears asymmetric and irregular, lacking a well-defined shape. There are hints of tidal tails or extended features stemming from the central regions, which further support the hypothesis of a galaxy merger or close encounter. The galaxy's color profile suggests a composite stellar population, with both older, redder stars concentrated in the core and younger, bluer stars populating the outer regions.
