The galaxy presents a generally smooth, elliptical morphology. Its central bulge is prominent, appearing largely spheroidal and concentrated, with a distinct yellow-orange hue. The light suggests an older stellar population within the bulge, potentially dominated by evolved red giant stars. The outer regions of the galaxy show a gradual decrease in surface brightness and exhibit a more diffuse distribution of light. There are subtle indications of a disklike structure faintly present, oriented roughly horizontally, however, any spiral arm features are absent or extremely faint. The galaxy is consistent with an evolved system, where star formation is substantially reduced. Minimal evidence of recent or ongoing major merger events is noted, but very minor disturbances or interactions cannot be ruled out given the faintness of the outlying regions.
