The galaxy presents a moderately luminous, disk-dominated structure with possible indications of a slight disturbance or interaction. The galaxy's light profile appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue. There is a central bulge or concentration of light, although it does not appear extremely prominent. Evidence of a disk component can be inferred, despite a generally smooth overall texture. The galaxy shows signs of ongoing, albeit moderate, star formation activity. Morphological classification suggests there is a higher likelihood of the galaxy not undergoing any major merging events, however, there is a possibility of a minor disturbance. Overall, the galaxy appears as a relatively massive, somewhat evolved system at a moderate distance, showing some low-level peculiarities in its structure.
