The galaxy appears as a flattened elliptical or lenticular structure. It exhibits a smooth, relatively featureless morphology. The central region is notably brighter, suggesting a concentrated nucleus or bulge. The color gradient transitions from a yellow-orange core to a greenish-blue periphery. This may indicate differences in stellar populations and/or dust content across the galaxy. The overall shape is elongated, appearing cigar-shaped rather than perfectly circular. There is no visual evidence of major mergers or significant tidal disturbances, although a slight asymmetry could hint at a minor interaction or internal dynamics. The general smoothness suggests a relatively quiescent star formation history, with a dominant population of older stars in the central regions.
