The galaxy appears as a relatively compact object with a smooth, elliptical morphology. The color profile suggests a higher concentration of older stellar populations, as indicated by the yellow-red hue. There is no obvious spiral structure or prominent dust lanes visible. The galaxy is elongated, appearing somewhat cigar-shaped. There are no indications of major mergers or strong tidal disturbances. The galaxy’s light profile appears regular and undisturbed, lending support to the classification of a relaxed system.
