The galaxy presents as a spiral type, viewed at an oblique angle, though without a clearly defined edge-on disk. It exhibits a moderately sized bulge region that contributes significantly to the galaxy's overall luminosity. While not readily apparent, subtle indications suggest the presence of spiral arm structures extending from the central bulge, though these are not sharply defined.

Color gradients are noticeable, with the central bulge exhibiting a yellowish hue, potentially indicative of an older stellar population. Fainter bluish regions are observed in the disk, suggesting pockets of more recent star formation.

No strong bar-like structure is discernible within the central region. There is no visual evidence to suggest any ongoing major merger events, though some minor asymmetries or disturbances in the outer disk cannot be completely ruled out based on this image alone.
