The object presents as a spiral galaxy with a discernible disk structure. Spiral arms are visible, exhibiting a moderate-to-tight winding pattern. The galaxy's central bulge appears relatively small compared to the overall disk size and exhibits a yellowish hue, potentially indicative of an older stellar population. The spiral arms show a bluer color, suggesting ongoing star formation. Dust lanes may be present within the spiral arms, though image resolution limits clear identification. There are no obvious signs of a strong bar structure. There is a slight suggestion of interaction, but the system is relatively undisturbed. Overall, this galaxy appears to be a relatively normal spiral galaxy with moderate star formation activity and a stable disk structure.
