The galaxy appears as a diffuse, elliptical object with a bright central bulge. The core exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the center, the light becomes bluer, indicating the presence of younger stars and perhaps ongoing star formation. The galaxy lacks a well-defined spiral structure, showing instead a more amorphous, disturbed morphology. Faint extensions or tidal features are potentially visible, hinting at past or ongoing interactions with another galaxy, or recent merger activity. Overall, the galaxy seems to be undergoing some kind of disturbance, but it could also simply be a transitional stage from a spiral to an elliptical. Further observation would be needed to determine this.
