The galaxy presents as a disk-shaped system with a concentrated central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. The surrounding disk is fainter and displays a bluer color profile, potentially indicating ongoing star formation. The disk appears relatively smooth with some subtle irregularities. There is a faint disturbance, suggesting minor interaction. Overall, the galaxy does not exhibit strong spiral arm structure. The galaxy appears to be an intermediate type between a lenticular and a spiral.
