The galaxy appears as a centrally concentrated, ellipsoidal object with a smooth morphology. Its core exhibits a yellowish hue, potentially indicative of an older stellar population. Extending outward from the core, a more diffuse envelope is visible. There is a slight asymmetry in the galaxy's overall light distribution, with a subtle extension or tail-like feature emerging on one side. Given its smooth appearance and elliptical shape, this galaxy is likely an elliptical or lenticular type. It exhibits a morphology consistent with a quiescent galaxy, not displaying any prominent spiral arms or significant dust lanes. The faintness of the outer regions suggests a gradual decline in stellar density moving away from the galactic center.
