The galaxy presents a generally smooth, elliptical morphology. There's a centrally concentrated brightness gradient, appearing more luminous towards the core. The galaxy exhibits a yellow-reddish hue overall, which may indicate an older stellar population and suppressed recent star formation, with dust possibly contributing to the redder colors. The light distribution suggests the system is largely spheroidal, lacking prominent spiral arms or a well-defined disk structure. There are no clear indications of tidal features or major disturbances in the image, suggesting it is not currently undergoing a major merger, although there may be some minor disturbances to the morphology.
