The galaxy presents as a somewhat elongated, disk-like structure oriented approximately horizontally in the image frame. Its overall color is a mix of blue-white and red-orange hues. The blue-white component appears to be more dominant on one end of the galaxy, suggesting regions of recent or ongoing star formation. This area is also slightly brighter and less diffuse, possibly indicating a higher concentration of young, hot stars. In contrast, the opposite end exhibits a more diffuse and red-orange coloration, which may be indicative of an older stellar population. The galaxy appears relatively smooth with no distinct spiral arms or bulges discernible at this resolution. There may be minor signs of tidal disturbance on the fainter edge of the galaxy, indicating potential interactions with other galaxies. Overall, the galaxy presents a fairly regular shape with subtle color variations suggestive of varying stellar populations and star formation activity within its structure.
