The galaxy presents as a relatively smooth, elliptical form. Its overall shape is cigar-shaped, displaying a noticeable elongation, but not extremely so. The light distribution suggests a concentration of older stellar populations. The central region exhibits a yellowish hue, possibly indicative of older stars and a lack of significant dust obscuration. The outer regions are fainter, and there is a slight blue tint in the galaxy's outer disk, suggesting some regions of lower star formation. There are no prominent spiral arm structures or clear signs of active star formation regions discernible. No strong tidal features or significant signs of an ongoing or recent major merger event are visually apparent. A slight asymmetry in the outer regions can be seen.
