The galaxy exhibits a moderately disturbed morphology, appearing as a fuzzy central bulge with some extensions suggesting tidal features or ongoing interactions. The central region displays a yellowish or reddish hue indicative of older stellar populations, possibly dominated by evolved stars. Fainter blue patches are visible in the outer regions, suggesting pockets of ongoing star formation, but likely at a relatively low rate. The galaxy is not perfectly smooth, with some irregularities in its light distribution, likely due to the interactions. The shape is generally elongated, but it does not possess a strong disk-like structure. There is evidence of a potential merger or strong interaction occurring, given the distorted shape and tidal features. This galaxy is a prime candidate for a study of merging galaxies and their impact on stellar populations and star formation.
