The galaxy presents as a relatively smooth, elliptical or lenticular structure with a prominent, bright central bulge. The overall color appears to be yellowish, suggesting an older stellar population with lower rates of ongoing star formation. There is a slight elongation, but the galaxy is mostly observed as having an intermediate shape. There are subtle hints of a disk, but not highly pronounced. A possible minor disturbance is observable in the main body of the galaxy, indicating a possible interaction with another galaxy. The galaxy does not obviously show evidence of ongoing, major merging activity.
