The galaxy presents a predominantly smooth morphology. Its shape is generally round, with no obvious spiral arm structures visible. A bright, concentrated central bulge is apparent, dominating the overall luminosity. The color gradient suggests a higher concentration of older stellar populations in the central regions, shifting toward slightly bluer hues in the outer regions. There is no obvious evidence of ongoing major mergers or significant tidal disturbances within the visible structure of the galaxy. The outer halo appears diffuse and relatively faint.
