The galaxy presents a generally smooth appearance, with a slight elongation along its major axis, giving it a somewhat cigar-shaped form. A central bulge is discernible, appearing brighter and more concentrated than the outer regions. There's a suggestion of a disk-like component, though it appears largely featureless, lacking prominent spiral arms or distinct dust lanes in this imaging. The galaxy's color is predominantly bluish, possibly indicating a population of relatively young, hot stars contributing to its overall light output. There might be some minor disturbances in its structure, but no clear indication of a recent major merger event can be seen. The overall impression is of a disk galaxy with a dominant bulge and a smoothly distributed stellar population.
