The galaxy presents a mostly smooth morphology, but with some indication of disk-like or featured structure. Its shape is elongated, resembling a cigar shape. The color profile suggests a bulge that is yellower, potentially indicating an older stellar population. There seems to be a faint, bluer region around the galaxy, suggesting the possibility of lower-level star formation. There is no evidence of any recent major merging activity, but there may be minor disturbances present. Overall, this is an older massive galaxy at intermediate distance, but still has ongoing lower-level star formation.
