The galaxy presents a relatively smooth morphology with a predominantly round shape. There appears to be minimal or no distinct spiral arm structure. The light distribution suggests a centrally concentrated spheroid. The galaxy exhibits a blue-white hue, suggesting the presence of a young stellar population, although the smoothness may indicate an older galaxy. There are no apparent signs of major mergers or significant tidal disturbances, but a very faint irregularity could indicate a minor interaction or internal activity.
