The galaxy presents as a relatively smooth, centrally concentrated object, suggestive of an early-type morphology. Its overall color is yellowish, indicative of an older stellar population with lower levels of ongoing star formation. The shape appears generally elliptical, with a subtle elongation. There is no obvious spiral arm structure or significant dust lane features visible within the resolution of the image. There are no signs of strong tidal disturbances or ongoing merger activity. The galaxy appears to be relatively isolated with no close companions that would indicate gravitational interactions.
