The galaxy appears as a centrally concentrated object with a relatively smooth profile. The central region exhibits a bright, almost unresolved core, indicative of either a dense stellar population or potentially an active galactic nucleus. Surrounding this core is an extended halo, which displays a greenish-blue hue, possibly indicating ongoing star formation. Faint reddish patches are present on the outskirts of the object, which may suggest regions of older stellar populations or dust obscuration. Overall, the galaxy appears to be an elliptical, rather than a spiral, and exhibits a relatively regular morphology.
