The galaxy presents as a moderately inclined disk system. A central bulge is clearly visible, exhibiting a yellowish hue, potentially indicating an older stellar population. The disk component displays a subtle color gradient, transitioning from a slightly greenish tinge near the bulge to bluer tones in the outer regions, suggestive of ongoing or recent star formation in those areas. The overall shape appears somewhat elongated, not perfectly circular. There is no clear evidence of strong spiral arm structures or significant tidal disturbances, however, some minor asymmetry might be present in the disk. The galaxy appears relatively smooth, with a high degree of central concentration of light.
