This galaxy presents a complex morphology. The central region exhibits a smooth, diffuse appearance, suggesting a spheroid-like structure possibly dominated by an older stellar population. Extending outwards from this core is a fainter, more irregular structure. There appears to be a slight blueish tint to the galaxy indicating the possible presence of younger stars.  Furthermore, hints of tidal features or minor disturbances are observed, possibly indicating a past or ongoing interaction with another galaxy.  Given the overall shape and the features observed, this system could be the result of a recent or ongoing merger, exhibiting characteristics of both elliptical and irregular galaxy types.
