The galaxy presents as a somewhat elliptical structure with a smooth, featureless appearance, suggesting a likely classification as an elliptical galaxy, though the presence of a disk component cannot be entirely ruled out due to the observed shape. The central bulge region exhibits a yellowish-orange hue, indicative of an older stellar population with relatively little ongoing star formation and a prominence of redder giant stars. Moving outwards from the center, the light gradually diminishes. The absence of distinct spiral arms or prominent dust lanes further supports the characterization of this galaxy as evolved, with a potentially low specific star formation rate. There are no signs of any active galactic nuclei or merger activity based on the image provided, which is consistent with the high smooth fraction of the morphology. The aspect ratio suggests a noticeable, but not extreme, degree of ellipticity.
