The galaxy appears to be a flattened spheroid, elongated along one axis, suggesting it is likely an elliptical or lenticular type. There is a concentration of light towards the center, indicating a nucleus. The light is broadly distributed and has a smooth appearance, with no prominent spiral arms or distinct features immediately apparent. The galaxy exhibits a subtle color gradient, shifting from a bluer hue towards the outer edges to a redder hue towards the center. The observed color profile may be indicative of differences in stellar populations, or dust content. There is no evidence of major ongoing merger activity or significant tidal disturbances in this image.
