The galaxy presents a somewhat amorphous structure, lacking a well-defined spiral arm morphology. The central region appears to exhibit a relatively smooth light distribution with a subtle central bulge. There is evidence of ongoing or recent star formation, indicated by the presence of bluer regions within the galaxy's disk, particularly in the areas surrounding the core. These blue regions may correspond to areas with younger stellar populations. The outer regions of the galaxy seem to fade gradually into the background, suggesting a less dense distribution of stars and gas. The overall structure shows some irregularity, possibly indicative of past interactions or mergers. The galaxy exhibits a faint reddish hue in some areas, potentially signaling the presence of older stellar populations and dust.
