The galaxy presents an overall elliptical shape, with a smooth, featureless appearance dominating its morphology. There is a noticeable color gradient, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population and diminished star formation activity in the core. Fainter greenish hues around the periphery suggest a bluer stellar population compared to the core. The light distribution shows a relatively smooth radial profile, with no distinct spiral arm structures or prominent dust lanes visible. The galaxy exhibits a moderate redshift, suggesting that the light we observe has been stretched as it traveled across vast cosmic distances. The galaxy's angular size is small. It appears to be undergoing some form of disturbance event, possibly merging, indicating strong tidal forces are acting on this galaxy. 
