This galaxy presents as a near edge-on disc galaxy with an elongated, elliptical morphology. A distinct central bulge is visible. The bulge appears to be smoothly distributed, and lacks significant internal structure. The disk exhibits a flattened profile with an axial ratio less than 0.5, indicative of significant inclination to the line of sight. There is no evidence of spiral arm structure.

The galaxy exhibits a radial color gradient, transitioning from a yellowish-white hue in the central bulge to a bluer color in the outer disk. This could indicate ongoing star formation in the outer regions. There is no evidence of dust lanes.

The overall appearance suggests a relatively evolved system with a dominant bulge component. Based on the edge-on morphology, accurate assessment of internal structure is challenging. There is no evidence of any strong tidal features or disturbances, suggesting that the galaxy is not currently undergoing a major merger or strong interaction.
