The galaxy appears to be a relatively smooth, elliptical system. There is an apparent concentration of light towards the central region, suggesting a bulge. The galaxy exhibits an elongated shape, possibly cigar-shaped, without any immediately obvious spiral arms or prominent disk features. Overall, the morphology appears undisturbed, with no indications of major mergers or tidal interactions. The color profile shows a concentration of redder hues toward the galaxy's core, possibly indicating an older stellar population, with the outer regions exhibiting slightly bluer tones.
