The galaxy presents as a centrally concentrated, relatively smooth object with an elliptical morphology. The core region exhibits a bright, intense luminosity, which gradually decreases towards the outer edges. A subtle blue hue characterizes the galaxy, particularly pronounced in the immediate vicinity surrounding the core. This suggests the presence of younger stellar populations, even though the overall smooth morphology suggests that the galaxy is an older system. There are no visually distinct spiral arm structures or prominent dust lanes are observed, supporting the idea of a mostly smooth structure. There may be some evidence of minor disturbances but there is no visual evidence of a major merger. The galaxy displays a moderate degree of roundness, not appearing highly elongated. The general appearance indicates a system undergoing relatively low levels of star formation. 
