The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. There is a slight elongation in its shape, but it is mostly rounded. The galaxy exhibits a concentrated central bulge that gradually fades into the outer regions. No prominent spiral arms or distinct dust lanes are visible. The color profile suggests a relatively older stellar population. The galaxy exhibits a weak, diffuse halo surrounding the main body. There is a possibility of minor interaction or disturbance, although the galaxy seems to be fairly isolated.
