The galaxy presents as a relatively smooth, centralized concentration of light. The morphology appears largely elliptical, exhibiting a high degree of central concentration with a radial decrease in luminosity. The color is predominantly yellow/orange, indicative of an older stellar population, and a lack of significant on-going star formation. There is no prominent disk structure visible and no strong evidence of spiral arms. The galaxy appears undisturbed, showing no signs of major mergers or tidal interactions. Any potential merger events would be classified as minor disturbances, if present. The isophotes appear fairly regular, further supporting the interpretation of a relaxed, dynamically evolved system.
