The galaxy presents as a single, relatively smooth, and concentrated object with an overall elliptical appearance. The color profile suggests a dominant population of older stars, with a moderate presence of younger stellar populations. Evident within the galaxy's morphology is an ongoing merger event with a smaller interacting companion. This interaction is characterized by a minor disturbance in the primary galaxy's structure. The overall luminosity implies a moderately massive galaxy, and with an inferred moderate rate of star formation.