The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The overall shape is elongated, though tending toward round rather than cigar-shaped. The color profile indicates an older stellar population, evidenced by the yellow-red hue dominating the galactic body. The light is evenly distributed throughout the galaxy with only a slight gradient towards the core, suggesting a lack of significant ongoing star formation. There appear to be no strong indicators of major mergers or significant tidal disturbances affecting the overall structure, though some very minor asymmetries may be present in the outer halo.
