The galaxy appears as a relatively small, moderately luminous object with a slightly elongated, cigar-shaped morphology. The central region exhibits a smooth, diffuse glow, with no distinct nucleus immediately apparent. A faint, disk-like structure extends from the central bulge. The overall color suggests a stellar population that is not particularly young or actively forming stars. There are no obvious signs of ongoing mergers or tidal disturbances, although a subtle asymmetry within the faint disk hints at possible past gravitational interactions. The galaxy's structure is somewhat disorganized, lacking well-defined spiral arms or a strong bar.
