The galaxy appears to be a spiral type, although the image resolution makes it difficult to discern fine details. There's a bright central bulge exhibiting a yellowish-white hue, which likely indicates an older stellar population. Fainter, bluer arms extend outwards from this central region, suggesting ongoing star formation. The disk is not particularly well-defined, possibly indicating some degree of disturbance or interaction. The overall structure shows some asymmetry, potentially due to a past or ongoing minor merger event. The galaxy seems to exhibit a moderate amount of star formation and a mass slightly above average for the galaxies observed in our studies. 
