The galaxy appears as a slightly elongated, disk-shaped object, viewed at a moderate inclination. The central region exhibits a significantly brighter concentration of light, suggesting the presence of a substantial galactic nucleus. The overall color profile of the galaxy tends towards a redder hue, however, the nucleus emits light in the green spectrum. Some minor features are visible, however no distinct spiral arm structure is clearly discernible. The galaxy shows no obvious signs of major tidal disruption or ongoing merger events. The estimated effective radius of the galaxy appears to be around 2 kpc. The galaxy seems to be a relatively massive system, but its rate of star formation is very low.
