The galaxy appears as a centrally concentrated system with a generally smooth morphology, presenting an elliptical or lenticular-like structure. Its core is visibly brighter and more yellow, suggesting a population of older stars. The outskirts of the galaxy are more diffuse, with a color that appears to be a mixture of yellow, green, and red, possibly indicating regions of moderate star formation activity or the presence of a mixed stellar population. There are no obvious spiral arms or strong dust lanes visible. There is no evidence of a major ongoing merger. The overall color and apparent morphology are consistent with a galaxy at an intermediate redshift. There is a slight hint of minor disturbance.
