The galaxy presents as a somewhat smooth, elliptical structure with a notable ring-like feature encircling the central region. The main body exhibits a diffuse glow, likely a composite of starlight from a large population of older stars. The color distribution within the primary structure appears relatively uniform, suggesting a well-mixed stellar population with limited recent star formation. However, the circular structure is not well defined and contains multiple different sections with different colors.

The observed ring structure appears as distinct regions of red, green, and blue emission, indicating the presence of different populations or processes. The red emission may be indicative of older stars and/or dust, while the green and blue emission could point to regions of active star formation, suggesting a higher concentration of younger, hotter stars.

The overall appearance indicates a galaxy that is relatively isolated, without significant signs of ongoing mergers or tidal interactions.
