The galaxy presents a generally elliptical morphology. It appears to be largely smooth in structure, with a high concentration of light toward the center and a gradual decrease in surface brightness moving outwards. The galaxy exhibits a slight yellow-orange hue, suggestive of an older stellar population. There is very little evidence of spiral arms or other distinct features such as dust lanes. The galaxy appears undisturbed, with no signs of ongoing or recent major merger activity, though there may be minor disturbances. It appears moderately round, showing a slight elongation but deviating little from a circular form. The faint color suggests that the rate of new star formation is quite low.