The galaxy presents as a smooth, elliptical-like object with a concentrated, bright central region. Its morphology appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. The overall color profile suggests a population of older stars, with a general lack of intense blue star formation regions typically associated with younger stellar populations. There is a slight elongation in the galaxy's shape, but it is predominantly rounded. While subtle color variations exist, the galaxy lacks prominent dust lanes or spiral arm structures. Based on these characteristics, this galaxy likely possesses a relatively low specific star formation rate, and has a high probability of being a smooth, evolved system.
