The object presents as a relatively small, disk-shaped galaxy with a distinct, nearly edge-on orientation relative to our line of sight. The central bulge appears bright and concentrated, exhibiting a nearly uniform white color indicative of an older stellar population. A faint dust lane is visible along the equatorial plane of the galaxy, appearing reddish-brown and silhouetted against the brighter central region. The disk component displays a bluish hue, suggesting the presence of younger, hotter stars, although this emission is not uniform throughout the disk. The outer regions of the disk appear diffuse, with a gradual decrease in brightness towards the edges. Faint tidal features are observed in proximity of the galaxy, suggesting the possiblity of a merger. Overall the galaxy lacks a grand, well-defined spiral structure, and exhibits a rather smooth morphology.