The galaxy presents as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. The core region appears bright, exhibiting a strong concentration of light. Moving outward from the core, there is a gradual decline in surface brightness. The color distribution suggests a potentially older stellar population with hints of younger star formation. The galaxy exhibits a blue hue, with a slight green tinge, which may indicate some on-going star formation. No distinct spiral arms or other pronounced features are discernible within the visible structure, and there is no substantial visual evidence for tidal disturbances or significant ongoing merger activity, although a minor interaction cannot be entirely ruled out. Based on its overall morphology and color, this galaxy is likely an early-type galaxy possibly still in its transition phase.
