The galaxy appears to be a single, relatively smooth structure. It is centrally concentrated, with a bright core that appears elliptical in shape. The color distribution suggests a primarily older stellar population, evidenced by the reddish-orange hue in the central regions. Fainter, bluer light is observed in the outer regions of the galaxy, suggesting the presence of younger, hotter stars. There is a hint of minor tidal disturbance in the form of asymmetry, although no clear merger is ongoing. Overall, the galaxy presents as a well-established and mostly undisturbed system, showing characteristics of ongoing, but relatively low, star formation.
