The galaxy appears as a relatively smooth, unresolved object with a slight yellowish hue, suggesting an older stellar population. Its morphology does not exhibit any prominent spiral arms or a distinct disk structure. The light distribution is centrally concentrated, indicating a possible bulge component. There may be some minor disturbance in its shape, possibly suggestive of past or ongoing interactions, but there is no conclusive evidence of major merging events. Overall, the galaxy presents as a spheroid-dominated system, possibly an elliptical galaxy at a significant redshift.
