The galaxy presents a generally smooth and rounded morphology, appearing as a single, relatively concentrated body of light. The core is noticeably brighter, exhibiting a yellowish hue that transitions into a fainter, more diffuse halo with tinges of green, and red at its periphery. There's no clear evidence of spiral arms or a prominent disk structure; instead, the light distribution appears relatively uniform across the galaxy's face, suggesting a predominantly elliptical or lenticular type. No significant tidal features or signs of ongoing mergers are readily apparent, indicating it is likely an isolated system, or any interaction is not significantly disruptive.
