The galaxy presents a moderately luminous, elongated morphology. Its primary structure appears smooth and featureless, lacking prominent spiral arms or a distinct central bulge when viewed at this resolution. The overall color profile suggests a relatively evolved stellar population, exhibiting a yellowish-red hue indicative of older stars. There is no obvious active galactic nucleus. The galaxy's shape is cigar-like, with a relatively narrow width compared to its length. Possible minor disturbances or interactions cannot be entirely ruled out, but there is no significant evidence of tidal tails, distorted shapes, or obvious merger events at the present time. 
