The galaxy presents an elongated, cigar-shaped morphology, with its major axis oriented roughly vertically in the image. The central region exhibits a bright, concentrated bulge characterized by a yellowish-orange hue, suggestive of an older stellar population and a relative lack of on-going star formation in the core. Moving outward from the center, the luminosity gradually decreases.

There is a distinct lack of well-defined spiral arm structure. Instead, a faint, diffuse disk appears to surround the bulge. The disk appears relatively smooth and lacks prominent knots of star formation, indicating either a passively evolving system or a relatively low rate of current star formation. The overall color of the disk appears slightly bluer than the bulge, suggesting a younger stellar population compared to the bulge. There is a single object to the lower left of the galaxy.
