The galaxy presents a generally elliptical morphology with a relatively smooth overall appearance. A bright, concentrated central bulge is visible, surrounded by a more diffuse and less luminous halo. The light distribution suggests a fairly evolved stellar population, with a color gradient indicating a higher concentration of older, redder stars towards the galaxy's center. No distinct spiral arms or significant dust lanes are apparent. The overall structure suggests an elliptical galaxy type, potentially with ongoing or recent minor merger activity causing subtle disturbances in the outer regions. The galaxy exhibits a moderate redshift, suggesting a considerable distance.
