The galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated shape. Its core exhibits a bright, concentrated luminosity, suggestive of a significant stellar population density. The overall color profile indicates a population of older stars, with a bias towards redder wavelengths, but there is indication of some star formation. The galaxy's morphology is largely undisturbed, with minimal evidence of recent or ongoing major merger events. There may be minor disturbance from an interaction with a nearby object, but there is no clear major disturbance. The size of the galaxy is moderate.
