The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology. The light profile suggests an older stellar population, with a predominantly yellowish hue. The galaxy presents as elongated, exhibiting a cigar-like shape. There is no obvious evidence of spiral arms or a prominent disk structure. The galaxy's overall appearance indicates a system that has largely undergone the process of merging, and does not appear to be experiencing any recent major interactions with other galaxies. There is little evidence of ongoing star formation.