The galaxy presents a predominantly elliptical morphology with a high degree of central concentration. The core region exhibits a bright, luminous appearance, indicative of a dense stellar population. Moving outwards from the core, the light gradually fades, and the isophotes become somewhat elongated with a moderate flattening. The overall color profile seems to be dominated by older stellar populations, suggesting a lower rate of recent star formation. There appears to be little discernible structure within the galaxy, such as spiral arms or prominent dust lanes, which aligns with its classification as an elliptical galaxy. The smoothness of the light distribution is indicative of a well-mixed and relaxed stellar system, rather than one undergoing significant tidal interactions or mergers.
