This galaxy exhibits a prominent disk structure, viewed at a moderate inclination angle. Spiral arms are clearly visible, extending from the central bulge. A strong central bar appears to bisect the bulge region. The bulge itself seems to be of moderate size relative to the disk, with some degree of prominence, but not excessively large. There appears to be no significant signs of ongoing major mergers or tidal disturbances, though minor irregularities in the disk's morphology may suggest some past interaction. The color distribution suggests the presence of both older stellar populations in the bulge and younger, bluer stars in the spiral arms, indicative of continued star formation.
