The galaxy presents as an elliptical morphology with a high degree of central concentration. There is a bright, prominent bulge, approximately 5 kpc in diameter, surrounded by a fainter, diffuse halo extending to about 15 kpc. The galaxy exhibits a generally smooth appearance, although there is some subtle evidence of disturbances in the outer regions. Color gradients suggest a relatively red population, with a possible indication of recent or ongoing merger activity. There are no clearly defined spiral arms or a prominent dust lane visible in the image. The galaxy is exhibiting a slow rate of star formation.
