The galaxy presents as a moderately bright object, exhibiting a largely smooth and somewhat elliptical morphology. The light distribution appears concentrated towards the center, indicating a defined nucleus or bulge component. There is a subtle color gradient, with the core appearing slightly yellower than the outer regions. This might suggest an older stellar population dominating the central area, with bluer, younger stars present in the outer regions, although this difference is not drastic. There is a very faint hint of a disk component, though it is not well defined. There does not appear to be any indication of active merging or major tidal disturbances, although there are some possible disturbances.
