The galaxy presents a smooth, elliptical morphology. Its shape is elongated, resembling a cigar. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer edges. The dominant color is reddish-orange, suggesting a population of older stars and a relatively low rate of star formation. There is no distinct spiral arm structure visible, nor any obvious signs of ongoing merging activity or major disturbance. Small traces of bluer features could indicate limited star formation activity within a disk.