The galaxy presents as a centrally concentrated object with a relatively smooth morphology. There is a slight elongation or asymmetry, but it appears predominantly featureless in terms of spiral arms or distinct structures. The color profile suggests a relatively evolved stellar population, exhibiting a generally redder hue, but is still exhibiting a level of star formation. The galaxy's apparent size is small, indicating a substantial distance. There's no obvious evidence of a major ongoing merger, although there is a possibility for some minor disturbances. The overall shape tends towards intermediate to rounded rather than cigar shaped. 
