The galaxy presents a spiral structure, though the arms are not sharply defined and appear somewhat flocculent. A central bulge is apparent but not overwhelmingly dominant, contributing moderately to the overall galactic luminosity. The disk is viewed at a slight angle but not entirely edge-on. Evidence of a bar structure is subtle but potentially present. The galaxy exhibits a range of colors, with a more yellowish hue concentrated in the central regions, possibly indicative of an older stellar population, and bluer tones present in the outer regions of the disk, suggesting ongoing star formation. There is no clear evidence of a major merger event, although subtle signs of disturbance or tidal interactions cannot be ruled out.
