The galaxy presents a flattened, elongated morphology suggestive of a disk galaxy viewed at an oblique angle. It exhibits a relatively smooth texture, with the central region appearing brighter and more concentrated, indicating a bulge component. The color gradient transitions from a yellowish-orange core to bluer hues in the outer regions. The observed color gradient implies potential variations in stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars populating the disk. There is a slight asymmetry in the outer disk, with subtle, possibly tidal features or minor disturbances that could indicate past or ongoing interactions, although no major merger events are evident. The galaxy appears moderately massive with an active, though not exceptionally high, rate of star formation. The relatively compact size suggests it is likely a smaller spiral galaxy or a larger dwarf galaxy.
