This galaxy appears to be a spiral galaxy, exhibiting well-defined spiral arms extending from a central bulge. The arms are tightly wound, indicating a relatively ordered structure. A prominent, yellow/orange-hued bulge dominates the central region, suggesting a significant population of older stars.

The spiral arms display a mix of colors, with regions of blue indicating ongoing star formation. Dust lanes are not clearly visible, but there is some mottling in the arms, likely due to dust obscuration and areas of higher star formation. The overall morphology suggests a galaxy undergoing active star formation, although not at an extreme rate. There is a slight visual asymmetry that may be attributed to minor gravitational interactions with other galaxies.
