The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears nearly spheroidal. The light profile decreases gradually from the bright nucleus outwards. The galaxy is largely featureless, with no apparent spiral arms or dust lanes visible in this image. There is a subtle color gradient from the center outwards; the central region appears bluer, suggesting the presence of a younger stellar population relative to the outer halo, which exhibits a redder hue. The overall round appearance and lack of prominent features suggests that if there was a merging event, it must have been a long time ago. There is evidence of minor disturbance, but it is not major. Overall the galaxy appears to be relatively inactive, with a low estimated star-formation rate based on the red color of the outer halo.
