The galaxy presents a predominantly smooth morphology, appearing as a concentrated central bulge or core surrounded by a less defined, extended halo. There is a slight asymmetry in the light distribution suggesting a possible minor gravitational interaction or disturbance. Color gradients are observable, with the central region exhibiting a warmer, more reddish hue indicative of an older stellar population. The outer regions are comparatively bluer, suggesting a more recent, ongoing episode of star formation. Overall, the galaxy seems relatively isolated, exhibiting a structure consistent with an early-type spiral or lenticular galaxy at a moderate redshift.
