The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decrease in intensity outwards. The core region displays a yellowish-orange hue, suggesting an older stellar population dominated by red giants. Fainter, diffuse bluish light surrounds the core, potentially indicating a small amount of recent star formation activity. No distinct spiral arms or bar structures are discernible. The overall shape is nearly circular, showing only a slight deviation from perfect roundness. There is no visible evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity.
