The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated, but largely rounded morphology. The light profile appears to be dominated by an older stellar population, exhibiting a yellowish-red hue, particularly in the central regions, suggestive of evolved stars. A small amount of bluer emission is visible in the outskirts of the galaxy suggesting some amount of ongoing star formation. There are also no signs of spiral arms or a bar. The galaxy appears relatively isolated, showing no clear signs of major tidal disturbances or ongoing mergers in this particular field of view. However, the presence of a faint, disturbed feature to one side suggests minor interaction or past merger event.
