The galaxy appears to be an elliptical type, exhibiting a generally smooth and featureless morphology. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus. The overall shape is relatively circular, with a slight elongation. There is a gradual decrease in luminosity from the core outwards, with no distinct spiral arms or bar structures visible. The color profile suggests a population of older stars, contributing to the yellowish hue. There may be evidence of minor gravitational disturbances, but the galaxy appears to be mostly undisturbed.