The galaxy presents a roughly lenticular morphology. The central bulge appears prominent and exhibits a yellowish hue, suggestive of an older stellar population and/or significant dust obscuration. A faint, disklike structure surrounds the bulge, but is not well-defined. There are hints of bluer regions within the disk. There is another galaxy within the image, it appears to be a dwarf galaxy that has a faint, blue haze about it. There appears to be no major distortions or tidal tails emanating from the galaxy, suggesting it is not currently undergoing a major merger, though subtle irregularities within the disk cannot be ruled out as signs of a minor interaction. 
