The galaxy presents as a moderately luminous, elongated structure, exhibiting a smooth, largely featureless morphology. The dominant color appears to be yellowish-white, potentially indicative of an older stellar population. The galaxy's shape is markedly cigar-shaped and the light is concentrated towards the center. There is little evidence of spiral arms, strong dust lanes, or distinct star-forming regions. The galaxy appears relatively undisturbed, with no major signs of recent or ongoing merger activity. It is estimated to be a moderate mass, with some ongoing star formation at a low rate.
