The galaxy presents as a moderately elongated, lenticular structure. It appears to have a relatively smooth overall texture, lacking prominent spiral arms or distinct features. The color gradient suggests potential variations in stellar populations, with a subtle shift towards bluer hues in the central regions. This could indicate ongoing, albeit moderate, star formation activity within that area. The galaxy has a redshift of around 0.2 and an estimated diameter of about 6 kpc, suggesting it's a relatively compact object at a substantial cosmological distance. A faint, disk-like structure may be present upon closer examination, giving it a more intermediate shape between elliptical and spiral. Signs of disturbance, possibly hinting at minor gravitational interactions or recent mergers, are possibly visible in its slightly irregular shape.