The galaxy presents as a somewhat elliptical object. The central bulge is bright and yellow-white, exhibiting a smooth, concentrated appearance, likely composed of an older stellar population. A fainter, bluer, and less-defined disk appears to surround the central bulge, extending along the galaxy's major axis. There are faint hints of some structure within the disk, but without clear spiral arm definition. The overall color profile suggests ongoing, but not exceptionally high, levels of star formation within the disk. There appears to be a minor asymmetry in the outer regions of the disk, potentially indicating a past minor interaction or merger event. No significant dust lanes are clearly visible. The galaxy does not appear to be a late-stage merger, and is rather quiescent.
