The galaxy presents a generally smooth, elliptical morphology. There is a bright central bulge with a diffuse halo that extends outward. The galaxy appears to be relatively isolated, with no obvious major tidal features or close companions to suggest a recent major merger, although there may be signs of minor disturbances in the outer regions. The colour profile suggests a relatively evolved stellar population, dominated by older, redder stars, particularly within the bulge. Some bluer regions may exist that possibly indicate ongoing or recent star formation at a low level. The object displays a noticeable degree of roundness in its overall shape, indicating it likely lacks a dominant disk structure.
