The galaxy presents as a generally smooth, elliptical-like structure, with a concentrated central bulge. There is a slight elongation, but overall, the galaxy appears largely rounded in shape. The color is primarily a yellow-orange hue, suggesting a population of older stars and a relatively low rate of recent star formation. There is little evidence of spiral arms or significant dust lanes. Some minor disturbance or a faint tidal tail may be present on one side, but it is not a prominent feature. The galaxy does not appear to be undergoing a major merger. 
