The galaxy presents an overall elliptical morphology. The central region exhibits a concentrated, smooth distribution of light, appearing yellowish in color. This suggests an older stellar population dominating the core. Fainter extensions are observed around the central region. These appear subtly blueish, hinting at the possibility of younger stars forming in the outer regions, although at a low rate, which seems to have caused some disturbance in its shape. There is no distinct spiral arm structure, but a slight asymmetry can be seen, giving it a "featured" look. A low-level interaction with a smaller galaxy may have occurred at some point.
