The galaxy appears to be a relatively compact object with a generally smooth morphology. It presents with a somewhat elliptical shape. There is a slight elongation, but the overall form is predominantly round. The color profile indicates a higher intensity in the red and far-red portions of the spectrum, which is suggestive of an older stellar population. There appears to be very little, if any, evidence of ongoing star formation within the galaxy. There are some faint, diffuse features near the center of the galaxy that might suggest a very minor disturbance or interaction, however it is most likely a static elliptical. The galaxy seems to be a well-defined, single structure with no clear signs of a recent or ongoing merger event.
