The galaxy exhibits a flattened, disk-like morphology, suggesting a spiral or lenticular type. A prominent, bright central bulge dominates the galaxy's core, characterized by a yellowish hue, which could indicate an older stellar population. Fainter spiral arm structures are suspected to be present. The disk appears moderately inclined with an inclination of approximately 25 degrees relative to our line of sight. The bulge's size appears moderate in relation to the overall dimensions of the galaxy. There is no obvious disturbance, indicating that the galaxy is likely an isolated galaxy that has not undergone a major recent interaction with another galaxy. The galaxy appears to be relatively isolated and not currently undergoing a major merging event.
