The galaxy exhibits a morphology that appears as a possible edge-on disk galaxy, characterized by a bright, yellowish central bulge. The bulge transitions into a fainter, elongated disk structure. The light distribution suggests a higher concentration of older stellar populations in the bulge, indicated by its yellower color. The disk presents a bluer hue, possibly indicating the presence of younger stars and ongoing star formation.

The disk seems somewhat disturbed or warped. There's an apparent asymmetry to the luminosity of the galaxy, indicating a possible tidal interaction or recent merger. The overall shape could be described as elongated with some disturbances in the disc's structure.
