The galaxy presents as a centrally concentrated system with an apparent smooth morphology. It exhibits a roughly elliptical shape, appearing mostly round. The core region displays a yellowish hue, transitioning to a faint bluish halo surrounding it, suggesting the presence of a mixed stellar population. There is no obvious evidence of spiral arm structure or a distinct disk component. No significant tidal features or other signs of ongoing major merger activity are observed. There is a slight asymmetry in the outer regions, which may be due to a minor disturbance or interaction, though more detailed spectroscopic data would be required to confirm this. The galaxy appears relatively isolated within the observed field.
