The galaxy presents an overall smooth appearance, suggesting an elliptical morphology or a lenticular disk galaxy viewed at a significant inclination. The central region exhibits a higher concentration of luminosity, appearing yellowish-white in color. This may indicate an older stellar population dominating the core. Extending outward from the center, the color transitions to a redder hue. The shape of the galaxy is elongated, with the ratio of its major to minor axis being quite substantial, close to 1:2 or even 1:3. No prominent spiral arm structures or dust lanes are visible. No apparent merging or tidal features, which may be indicative of recent or ongoing interactions with other galaxies, can be seen. There might be a slight warp in the disk.
