The galaxy presents a primarily smooth morphology, although subtle features suggestive of a disk or disturbance are discernible. A central bulge region exhibits a yellowish hue, indicative of an older stellar population. Extending outwards from this central region, are fainter, bluish areas implying the presence of younger, hotter stars or regions of active star formation. Overall, the galaxy appears somewhat elongated in shape. There may be a possible minor disturbance present in the galaxy. A small area of the galaxy is brighter than others.