The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated distribution of light. The core region displays a yellowish hue, potentially indicating an older stellar population. The galaxy is elongated and appears somewhat cigar-shaped. There is a subtle blue tinge in the outer regions, suggesting the presence of a younger stellar population, although the overall contribution of these stars to the total light output seems to be minimal. The galaxy displays no obvious signs of recent major mergers or significant tidal disturbances. There is also no prominent spiral structure.
