The galaxy presents as a cigar-shaped, elliptical morphology, with a smooth overall appearance lacking discernible spiral arm structures. It exhibits a bright, centrally concentrated core region that gradually fades toward the outer edges, consistent with a spheroidal distribution of stellar mass. The isophotes appear elongated, indicating a significant ellipticity. Color gradients suggest a potentially older stellar population with a slightly redder hue overall. There appears to be little to no dust obscuration visible within the galaxy's structure, contributing to its relatively smooth and featureless appearance. The light distribution is best described with a high Sersic index.
