The galaxy presents as an elongated structure with a relatively smooth overall appearance. There is a prominent central bulge that seems to be the brightest region. Emanating from this core are what appear to be arm-like features, however they are not well-defined or tightly wound. These arms fade into a more diffuse outer disk.

The color of the galaxy is predominantly blueish-white, particularly within the central bulge and the inner regions of the arms. This color suggests a significant population of young, hot stars, indicative of ongoing or recent star formation. There may be some indication of dust lanes or areas of obscuration within the disk.

There are potentially signs of minor disturbances in the galaxy’s structure. These could arise from a minor tidal interaction or some other gravitational disturbance. However, overall the galaxy appears to be relatively stable.
