The galaxy presents a primarily smooth morphology, with a notable elongation in its shape. The light distribution appears concentrated and centralized. The galaxy has a redder hue, possibly indicating an older stellar population and a lower rate of ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible. There are no clear signs of recent major mergers, though there might be some indication of minor disturbances. The galaxy is relatively compact in size, suggesting a moderately sized elliptical or lenticular galaxy at a considerable distance.
