The galaxy appears to be a spiral type, exhibiting a central bulge and fainter, elongated arms extending outward. The bulge is relatively bright and compact. The structure of the arms suggest possible disruption or tidal interaction, evidenced by their less defined and somewhat asymmetrical morphology.

The color gradient within the galaxy suggests varying stellar populations. The central bulge exhibits a yellowish hue, indicative of older stars. The outer regions and arms show hints of bluer colors, potentially signaling ongoing star formation. Overall, the galaxy shows evidence of both smooth structure and disturbed features.
