The galaxy presents as an elongated, likely elliptical or lenticular, structure. A prominent central bulge is visible, exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions appear fainter and bluer, suggesting the presence of a younger, star-forming population, albeit less pronounced. The galaxy exhibits a smooth texture, with no clear spiral arm structure or significant dust lanes visible in this image. The overall morphology suggests a system that is not currently undergoing a major merger or significant tidal disruption. It appears relatively isolated and undisturbed.
