The galaxy presents as a fairly elliptical object, with an observed axis ratio of approximately 0.6. The light profile appears concentrated toward the center, transitioning smoothly outward. The core exhibits a yellowish hue, suggestive of an older stellar population. The outer regions show a bluer tint, hinting at more recent or ongoing star formation. There is no obvious spiral structure; the overall morphology seems more akin to that of an elliptical or lenticular galaxy. The edges are indistinct, fading gradually into the background. There is a slight warp to the distribution of light, but this could be due to galactic interactions or an artifact of our viewing angle.
