The galaxy presents as a relatively face-on spiral, showing a prominent central bulge that dominates its visual appearance. The bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars in that region. Fainter and bluer spiral arms extend outwards from the central bulge, though their structure is somewhat indistinct and lacks sharp definition. The galaxy's overall color suggests a moderately evolved stellar population, with a mixture of older, redder stars in the bulge and younger, bluer stars in the arms. There appears to be some evidence of ongoing star formation within the spiral arms, as indicated by the presence of bluer regions, but the overall star formation rate seems moderate to low. The galaxy's shape appears somewhat elliptical. There are no obvious signs of a recent major merger or significant tidal disturbances, with the galaxy showing a relatively settled morphology.
