The galaxy presents as a moderately sized, relatively smooth object at a redshift of approximately 0.1. The light distribution appears concentrated towards the center, suggesting a possible elliptical morphology. A slight elongation is observed with a possible inclination. The galaxy exhibits a color gradient, transitioning from a generally bluer periphery to a redder core, which may indicate a radial difference in stellar populations with older stars closer to the center. There are no obvious signs of active star formation, and no major disturbances or mergers are apparent.
