The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a moderate amount of ellipticity. The color is predominantly yellowish, suggestive of an older stellar population. There is a fainter, smaller region visible on the upper left of the galaxy's core. This could be either a satellite galaxy or a region of star formation. There are very faint signs of disruption in the galaxy, which could indicate a recent merger, but is much more likely due to internal factors. Based on the size of the galaxy, it would be classified as a giant galaxy with considerable mass. 
