This galaxy presents as an elongated, cigar-shaped structure. The primary light emission appears concentrated towards the central region, exhibiting a yellowish-orange hue suggestive of an older stellar population. The outer regions display a gradual decrease in luminosity, transitioning to a bluish tint. This color gradient could indicate the presence of some younger, bluer stars in the outer regions.

The galaxy appears relatively smooth in texture, with no obvious spiral arms or dust lanes visible at this resolution. There may be a faint hint of asymmetry or minor disturbance in the morphology. The galaxy shows no clear signs of major ongoing merger activity. The estimated size suggests this is a moderately large galaxy.
