The galaxy presents as a generally elliptical form with a concentrated central bulge. The core appears to be a bright, yellowish-white, suggesting a relatively old stellar population and limited ongoing star formation in that region.

Moving outward from the core, the surrounding region exhibits a slightly bluer hue, hinting at the presence of younger, hotter stars or possible ongoing star formation in a disk feature that is nearly face-on with a slight inclination. There are subtle irregularities in the distribution of light throughout the disk, possibly indicating minor disturbances in the galaxy's structure.

The galaxy does not show any obvious signs of a recent major merger event, such as tidal tails or highly distorted morphology, but the slight asymmetry may imply some kind of merger that has occurred in the past. No dust lanes are clearly visible in this image.
