The galaxy presents a smooth, elliptical morphology. Its shape is elongated, appearing cigar-shaped rather than perfectly round. The color profile indicates a generally older stellar population, with a central concentration of reddish hues. There are hints of bluer regions in the outer parts of the galaxy, suggesting some degree of ongoing, albeit low, star formation activity. The overall structure shows no signs of major mergers or significant tidal disturbances. It appears to be a relatively isolated system with a dominant, smooth spheroid.
