The galaxy presents a somewhat amorphous structure, appearing neither distinctly spiral nor elliptical. Its overall color profile suggests a greater abundance of older stars, leaning toward a redder hue, though there are some bluer regions that could indicate younger stellar populations.

The light distribution within the galaxy is somewhat uneven, with a slightly brighter core region. There are faint, diffuse extensions or tidal features that suggest possible interactions with another galaxy. Morphological classification is made difficult by the apparent disturbance to the overall structure, making it challenging to determine the presence of spiral arms or a smooth elliptical profile. Further investigation would be needed to determine the galaxy's precise classification.
