The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge, which is bright and appears yellowish-orange in color. The light distribution fades gradually outwards, with the outer regions exhibiting a more diffuse, reddish-tinged glow. There is no clear evidence of spiral arms or a well-defined disk structure. The overall appearance suggests an evolved system, potentially with an older stellar population dominating the light output. No significant tidal disturbances or merging features are apparent, indicating relative isolation.
