The galaxy appears to be an elliptical galaxy, exhibiting a smooth, cigar-shaped morphology. It presents with a central bulge that dominates the galaxy's overall structure. The color gradient indicates a higher concentration of older stellar populations toward the central region, transitioning toward bluer colors in the outer regions. This suggests some ongoing, albeit low, levels of star formation activity. There's no clear evidence of spiral arms, or significant dust lanes and no indications of any major disturbances or recent merger events. 
