The galaxy appears as a slightly elongated, lenticular-shaped object with a relatively smooth light distribution. Its central region shows a moderate concentration of light. There is a subtle suggestion of a faint, diffuse structure potentially indicating a disk. However, this feature is not well-defined. The overall color profile indicates a population of older stars, as seen in the color profile skewing toward redder wavelengths. There might be a slight asymmetry or distortion in its shape, perhaps due to a minor gravitational interaction with a nearby object. Overall, this galaxy seems to be a relatively passive system undergoing no major starburst activity.
