The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution with a high degree of roundness.  The central region is notably brighter and presents a yellowish hue, suggesting an older stellar population.  Fainter, bluish-green emission is visible in the outer regions, potentially indicative of some ongoing, low-level star formation. There is no obvious evidence of spiral arms or a distinct disk structure. The overall morphology suggests a relatively relaxed system, without strong signs of recent major mergers or tidal disturbances, although some minor asymmetry cannot be entirely ruled out. The galaxy has an estimated size of a little over 6 kpc.
