The galaxy appears as a single, relatively smooth concentration of light. The overall shape is somewhat elliptical, tending towards round. The galaxy exhibits a yellow-red hue, indicative of an older stellar population. There is no clear evidence of spiral arms or significant dust lanes. Faint hints of diffuse light extend outwards from the central core, suggesting a gradual transition from the nucleus to the outer halo. There are no obvious signs of recent or ongoing merger activity, such as tidal tails or distortions in the overall shape. Based on the color and morphology, this galaxy is likely an elliptical galaxy at a moderate redshift.
