The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is minimal evidence of spiral arm structure or distinct morphological features. The light distribution appears relatively uniform, lacking prominent knots of star formation or significant dust lanes. The overall shape approximates an elliptical form, with a moderate ellipticity. The core exhibits a bright, slightly yellowish hue, indicative of older stellar populations. Fainter, redder light extends outwards from the center, suggesting a gradual decrease in stellar density and age with increasing radius. There is no obvious sign of a recent or ongoing major merger event. The low level of observable star formation aligns with the smooth, spheroidal appearance.
