The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. There is a dominant central bulge, which contributes most of the galaxy's overall luminosity. A slight elongation can be observed, though the galaxy is mostly round. There may be some minor disturbances in the overall structure, evidenced by slight asymmetry. There are some indications of potential star formation, as hinted by the faint blue tinge, although this appears to be limited. The red color of the central bulge indicates an older stellar population. Overall, the galaxy appears to be a massive system.
