The galaxy presents an elliptical morphology. Its light distribution appears relatively smooth and centrally concentrated, exhibiting a bright core. The galaxy appears to have a noticeable lack of distinct spiral arm structures or prominent dust lanes. The overall color is slightly reddish, suggesting an older stellar population and reduced recent star formation. There is a suggestion of a flattened spheroid, though the galaxy appears primarily spheroidal. No obvious signs of tidal disturbances, major mergers, or significant interactions with neighboring galaxies are apparent.
