The galaxy presents a mostly smooth, elliptical morphology. It exhibits a notable elongation, with a cigar-like shape. The central region displays a concentrated, brighter luminosity, suggesting a higher density of stars or potentially an active galactic nucleus. There is a color gradient from the center outwards, with the core appearing more yellow-white and the outer regions trending towards a redder hue, indicative of older stellar populations in the outskirts. There is little evidence of spiral arm structure, although slight disturbances might be present, but could be noise. The overall appearance suggests a relatively evolved galaxy with a low star formation rate.
