The galaxy presents as a generally smooth, elliptical-like object with a noticeable central bulge. The light distribution suggests a concentration of older stellar populations in the core, indicated by the yellowish-orange hue. Moving outward from the core, the galaxy gradually fades into the background sky. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy appears somewhat elongated, hinting at a possible deviation from a perfectly spherical shape. There are also subtle irregularities that suggest possible minor disturbances.
