The galaxy presents as a smooth, elongated structure, exhibiting a cigar-like morphology. The central region appears to be a high-density concentration of stellar material, possibly an aging stellar population, appearing more red than blue. The luminosity gradually decreases moving outwards from the center, with no apparent spiral arms or distinct features. The overall color suggests a galaxy dominated by older stars with a low rate of star formation. There is no evidence of major mergers or tidal disturbances in the image.
