The galaxy presents as a spiral with a moderately sized bulge. There is evidence of a bar structure across the central region. Indications of spiral arms are apparent but not sharply defined. The galaxy exhibits a notable central concentration of light, with the bulge appearing a yellowish hue. The disk, while partially obscured, appears to have a bluer tint, suggesting regions of on-going star formation. The overall structure appears relatively undisturbed, with no obvious signs of major merging activity, but there may be a slight asymmetry in its features.
