The galaxy appears as a centrally concentrated object, with a generally smooth morphology. The light distribution suggests a spheroid-dominated system, possibly elliptical or lenticular in nature, with a slight extension. The galaxy exhibits a color gradient, transitioning from a bluer hue at the center to redder outskirts. The overall color implies a substantial population of evolved stars, although the bluer central regions may indicate some ongoing star formation. There seems to be no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. It's axial ratio is close to one and the light is centered very closely to the redshift location.
