The galaxy presents as a moderately bright, elongated structure. Its morphology appears largely smooth, lacking defined spiral arms or significant dust lanes. The central region exhibits higher luminosity, indicative of a concentrated nucleus or bulge. The galaxy's color profile suggests a slightly bluer hue, especially toward the central region, potentially indicating ongoing star formation. A faint extension or tidal feature is suspected, but no other major mergers are visible. The overall shape is cigar-shaped, with a relatively smooth light distribution. 
