The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light distribution. It has a distinctly elongated, cigar-like shape. There is little to no evidence of spiral arm structures. The color gradient suggests an older stellar population, with a concentration of light in the redder wavelengths. There are no obvious signs of ongoing major mergers or significant tidal disturbances. Faint wisps or diffuse features are subtle indications of potential minor interactions or past activity. Overall, the galaxy presents as a relatively undisturbed, evolved system.
