The galaxy presents an overall elliptical morphology with a smooth, diffuse light distribution. A central bulge is apparent, exhibiting a higher concentration of light and a yellowish hue, possibly indicating an older stellar population. Moving outwards from the bulge, the galaxy exhibits a less concentrated, bluer component suggesting the presence of younger stars and ongoing star formation. There is a hint of a disk-like structure, with slight flattening observed along one axis. Minor disturbances and irregularities are visible in the outer regions, indicating a possible interaction or minor merger event in its past. Overall, the galaxy exhibits characteristics of a galaxy transitioning from a disk dominated galaxy, with a moderately high stellar mass and moderate to low levels of current star formation activity.
