The galaxy presents as a relatively smooth, concentrated structure. It exhibits a generally elliptical morphology, appearing quite round. The galaxy's light profile suggests a dominant bulge component, characterized by a yellowish hue indicating a population of older stars. There is little visual evidence of spiral arms or a distinct disk. The colors and morphology are consistent with an early-type galaxy, possibly an elliptical. There is some subtle color variation observed, with the central regions appearing more yellow and the outer regions trending toward a slightly bluer color. No signs of major mergers or strong tidal disturbances are immediately apparent. However, further spectroscopic analysis would be required to confirm this galaxy's exact composition and ongoing processes.
