The galaxy appears as a relatively small, yet moderately luminous object. It presents an overall elliptical shape with a discernible, albeit not sharply defined, disk-like structure. There's evidence of structural disturbance, possibly indicating an ongoing or recent interaction with another galaxy. This manifests as some asymmetry in the disk and perhaps some faint tidal features that could be plumes or tails extending from the main body. Based on the color distribution, the galaxy may contain both older stellar populations, visible as redder hues, and regions of active star formation, indicated by bluer tints within its structure. The galaxy doesn't appear particularly smooth.
