The galaxy presents as an elongated, cigar-shaped structure. Its overall color profile suggests a predominantly older stellar population. The central bulge appears bright and concentrated, exhibiting a yellowish hue, indicative of evolved stars. The disk component, while present, seems relatively subdued, lacking prominent spiral arm structures. Its color is slightly bluer than the bulge, possibly indicating some ongoing, albeit low, levels of star formation. There's no visually apparent evidence of major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed, exhibiting a smooth overall morphology. The absence of strong blue colors and prominent spiral features suggests a later-type galaxy, transitioning towards a more passive state of stellar evolution.
