The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge is apparent, exhibiting a slightly reddish hue. The surrounding halo appears more diffuse, with a subtle, faint greenish-blue tint, potentially indicative of some ongoing, though relatively low-level, star formation. There's no clear evidence of spiral arm structure or significant dust lanes. The overall shape is more rounded than elongated, suggesting a classification leaning towards E0-E3 on the Hubble sequence. There are no obvious signs of a major ongoing merger or significant tidal disturbances, although subtle irregularities might suggest minor interactions in the past.
