The galaxy appears as a collection of diffuse light, presenting an ill-defined morphology. Its color gradients suggest variation in stellar populations or dust content. The presence of multiple luminous areas, particularly the distinct orange region, indicates potential active star formation or a concentrated area of older stars. The overall faintness may suggest it is a low-mass galaxy, or that the star formation rate is slow. There is another brighter and bluer area, possibly indicating more star formation is taking place there. The overall appearance suggests a fairly smooth distribution of light, with no strong evidence of spiral arms or a well-defined disk. There is also a suggestion of minor gravitational interactions, but without higher resolution, this is difficult to assess.
