The galaxy presents as a late-type spiral, oriented edge-on relative to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. The galactic disk is clearly visible, extending outward from the bulge and displaying a bluer color, indicative of younger stellar populations and ongoing star formation. The disk appears relatively thin and without strong indications of spiral arm structure, likely obscured by the edge-on viewing angle. No obvious signs of a major merger event are visible, although there may be some minor asymmetry or disturbance in the outer regions of the disk. Overall, the galaxy exhibits a classical edge-on disk galaxy morphology.
