The galaxy presents as a relatively smooth structure with a concentrated central bulge. The morphology appears intermediate between elliptical and disk-like. The primary color observed is a yellowish-orange, suggesting an older stellar population dominating the light output. There may be some hint of a disk surrounding the bulge, although the structure is not clearly defined. The galaxy appears to be relatively isolated with no major signs of an ongoing or recent major merger. There may be a very slight disturbance, but if this is the case, it would be very minor.
