The galaxy presents a generally diffuse morphology, with a notable asymmetry in its structure. There appears to be a central bulge or core region, but it lacks sharp definition. Extending outward from this core are faint, irregular arms or extensions, suggesting the presence of disk-like features although not clearly defined. There is some indication of possible tidal disturbance or interaction, as the distribution of light is not smooth and continuous; there are some hints of disruption in its shape. The color suggests that the galaxy contains a mix of stellar populations, with some regions exhibiting bluer hues, indicative of ongoing or recent star formation, and other regions appearing redder, suggesting older stellar populations. Areas of redder concentration may correspond to dust lanes or regions of high gas density.
