The galaxy presents a generally smooth morphology. Its shape is elongated, but not drastically so, appearing somewhere between round and cigar-shaped. The central region is characterized by a bright, concentrated core that emits strongly in the redder wavelengths, suggesting an older stellar population or significant dust obscuration. A surrounding, less intense halo extends outward, displaying a gradient from yellow-orange towards greener hues. There is very little evidence of spiral arm structures or tidal tails, but a small portion of the galaxy seems to be slightly disturbed, though not obviously undergoing a major merger.