The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse morphology with a noticeable elongation. The overall color profile is yellowish, becoming more intense towards the central region, suggesting a concentration of older stellar populations. Faint, greenish hues are present surrounding the bright yellowish center, and it is possible that this indicates the presence of some star formation. No spiral arms or distinct features of a disk galaxy are discernible. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity that might suggest strong gravitational interactions.
