The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. There is little evidence of spiral arms or significant dust lanes. Its overall shape is somewhat elongated. Color gradients across the galaxy seem minimal, suggesting a lack of significant ongoing star formation. The galaxy does not appear to be undergoing any major mergers or interactions, although a slight asymmetry could indicate a minor disturbance in its past. Its light is relatively red, typical of older stellar populations.
