The galaxy presents as a generally smooth, elliptical form, elongated in shape with a cigar-like appearance. The central region exhibits a concentrated, bright core, suggesting a higher density of stars and potentially a supermassive black hole. Surrounding the core, the galaxy fades outwards in luminosity, displaying a gradual decrease in stellar density.

While generally smooth, subtle features suggest some internal structure, potentially faint disk-like components. There are no obvious signs of strong spiral arms or a well-defined disk. No major tidal distortions or interactions with companion galaxies are readily apparent, although minor disturbances may be present.

The color profile indicates an aging stellar population, with the light appearing redder overall. This suggests a lack of significant ongoing star formation.
