The galaxy appears as a relatively smooth, luminous structure. The central region exhibits a concentrated, yellow-orange hue suggesting an older stellar population. The galaxy's overall shape is somewhat elliptical, although not perfectly spherical. A slight asymmetry is observable, though it does not appear to be indicative of a major merger event. The absence of prominent spiral arms and the overall color profile suggests an early-type galaxy. There may be some ongoing, but limited, star formation activity. There is little evidence of significant dust lanes or recent tidal disturbances.
