The galaxy presents as an elongated, diffuse structure, with a significant degree of ellipticity. A bright, concentrated core region is discernible, exhibiting a smooth, featureless appearance. Moving outwards from the core, the galaxy's luminosity decreases gradually, resulting in a faint and extended halo or envelope. The overall color is bluish, suggesting a population of relatively young, hot stars. There is a hint of an irregular structure or possible tidal feature extending from the main body, indicating a potential interaction with another galaxy or recent merger event. It is difficult to discern any distinct spiral arms or well-defined features within the disk, if present. The galaxy's morphology appears to be transitioning towards a more spheroidal or elliptical shape.