The galaxy presents as a diffuse, moderately sized object. It lacks a distinct central bulge, exhibiting a more amorphous structure. The color gradient suggests varying stellar populations and dust distribution throughout the galaxy. The dominant color appears to be a slightly bluer hue, particularly in the central regions, implying the presence of younger, hotter stars. However, there are also redder concentrations, potentially indicating older stellar populations or regions obscured by dust.

There is evidence of disturbances in its structure. A significant portion of the light appears irregular. Patches of brighter emission are not symmetrically distributed, possibly indicating on-going interactions or recent merger events. Though a disk-like structure is not apparent, the observed features suggest at least minor gravitational interactions are contributing to the overall morphology. I also note a tidal tail on the left, likely resulting from a past merger event.
