This galaxy appears to be a spiral galaxy exhibiting a bulge. The bulge presents as a bright, concentrated region towards the center of the galaxy, and its light appears somewhat yellow-white.

Surrounding the bulge, the galaxy displays what appears to be spiral arms, although the arm structure is not clearly defined. These arms have a patchy, flocculent appearance, with some areas showing concentrations of bluer light, suggestive of star formation regions. The galaxy's disk is inclined at a moderate angle relative to our line of sight. There may be evidence of minor gravitational disturbances in the spiral arms. Overall, the galaxy shows a notable population of both older stars in the bulge and regions of ongoing star formation in the arms.
