This galaxy presents as a spiral type, viewed at an angle that is neither perfectly face-on nor edge-on. There is evidence of spiral arm structure, with hints of possibly three distinct arms emanating from the central region. The arms appear moderately wound, neither tightly coiled nor very loosely structured. A central bulge is discernable; it appears to be moderate in size relative to the overall galaxy, not overwhelmingly dominant but also not negligible. The color distribution suggests active star formation. The spiral arms exhibit bluer hues, likely indicative of younger stellar populations, while the bulge region is more yellowish, which can be associated with older, redder stars. The disk is not perfectly smooth; there is a notable amount of irregularity, perhaps due to ongoing or recent interactions. There is a possibility of a slight disturbance in the disk, but not indicative of a major merger event. The galaxy does not show strong bar structure in the central region.
