The galaxy presents a somewhat amorphous structure, exhibiting characteristics that fall between a smooth elliptical and a disk galaxy with visible features. The central region displays a concentrated, yellowish hue, suggestive of an older stellar population. Moving outward from the core, a faint bluish halo is observed, indicating the presence of younger stars and possibly ongoing star formation. 

There's a hint of disturbance in the overall shape, perhaps suggesting past or ongoing interaction with another galaxy. Though no distinct tidal tails or bridges are immediately apparent, a slight asymmetry hints at gravitational influence. Furthermore, the galaxy's extended, diffuse nature and the presence of blue light suggests active star formation.
