The galaxy appears as a centrally concentrated, relatively smooth structure with a slightly elliptical morphology. The core exhibits a bright, reddish-yellow hue, suggesting an older stellar population. The outer regions display a fainter, bluish tint, which might indicate the presence of younger, hotter stars, although this could also be influenced by redshift. There is some evidence of subtle disturbances or faint features in the disk, possibly suggestive of a minor interaction or internal dynamics. The galaxy lacks a strong spiral arm structure or prominent dust lanes, exhibiting a more diffuse appearance. Overall, the galaxy presents characteristics consistent with an early-type spiral or possibly lenticular galaxy at a moderate redshift. The estimated size suggests it is a relatively small galaxy, possibly a dwarf.
