The galaxy appears to be a relatively compact, elliptical-like system. It exhibits a smooth, centrally concentrated light distribution, lacking prominent spiral arms or distinct features. The morphology suggests a spheroid-dominated structure. The galaxy appears to be somewhat elongated, exhibiting a cigar shape. There is no obvious evidence of a major merger or significant tidal disturbance.

The galaxy shows a blue-ish hue in its core, and its outer regions have a slightly redder color, suggesting a difference in stellar populations or dust content between the core and the outskirts. The size of the galaxy is modest, typical for galaxies at its redshift. The estimated rate of star formation is relatively low.
