The galaxy presents as a somewhat elliptical, reddish object. Its overall form is relatively smooth, with no readily apparent spiral arms or significant dust lanes visible in this imaging. The central region exhibits a higher surface brightness than the outer regions, suggestive of a concentrated stellar population, possibly a bulge. There is very little blue light apparent, likely indicating an older stellar population with suppressed star formation. There is a minor suggestion of disturbance in the outer regions. The object is considered to be reasonably isolated, with no apparent major merger events in progress.
