The galaxy presents as a generally smooth and rounded object with a concentrated central bulge. It exhibits a yellow-white hue, which is suggestive of an older stellar population dominating the light output. The light distribution appears relatively uniform without prominent spiral arms or distinct features, indicating a more elliptical or lenticular morphology. There is a subtle color gradient, with the central regions appearing slightly more yellow/gold than the outer regions. The outer regions are less defined and dimmer than the center and display a subtle blue-ish tinge, hinting at a small amount of recent star formation compared to the core. There is no evidence of a major ongoing merger or significant tidal disruption, however there may be a minor disturbance in the galaxy's form. The galaxy is reasonably compact for its redshift.
