The galaxy presents as a relatively smooth, elongated structure. Its shape is significantly cigar-shaped. No distinct spiral arms or a prominent central bulge are clearly visible. There appears to be a concentration of light toward the galaxy's core, although it is not intensely bright. The overall color suggests a mix of stellar populations, with a possible dominance of older, redder stars, which would correspond with low star formation. There is no indication of significant tidal disturbances or ongoing mergers, but a minor interaction or disturbance cannot be entirely ruled out.
