The galaxy presents a generally smooth, elliptical morphology. It appears moderately luminous, with a concentrated central bulge that dominates the light profile. The outer regions exhibit a gradual decline in surface brightness, lacking distinct spiral arm structures or prominent features. The color profile suggests a population of older stars, with a yellowish-red hue characteristic of evolved stellar populations. There is no noticeable dust lane or evidence of significant ongoing star formation within the central region or outer disk. The overall form indicates a system that is most likely an early-type galaxy undergoing minimal interaction with other galaxies. It is moderately sized. Based on its appearance, it could be undergoing a minor disturbance.
