The galaxy presents as a relatively smooth, elliptical morphology. Its light profile is concentrated toward the center, with a gradual decline in brightness towards the outer regions. The galaxy exhibits a subtly elongated shape, deviating slightly from a perfect sphere. There's no evidence of prominent spiral arms or a well-defined disk structure, suggesting it is not a spiral galaxy. The galaxy has an estimated effective radius of approximately 3.2 kpc, indicating a moderately sized system. Color gradients are observed, with a redder hue towards the central regions. There is no obvious sign of active galactic nuclei activity or star formation within the galaxy. The overall appearance indicates a likely evolved system. There is no sign of tidal disruption or merger activity. 
