The galaxy presents an overall elliptical morphology. The central bulge exhibits a concentrated, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the disk displays a bluer color gradient, indicating the presence of younger, hotter stars. This could also mean more active star forming regions. The galaxy appears elongated, but there's a slight hint of a disk structure, hinting at a possible spiral component, though it lacks defined spiral arms. There's no obvious evidence of a major ongoing merger or tidal disturbance, but some slight asymmetry exists in the outer regions of the disk, suggesting a possible minor interaction. The overall appearance is relatively smooth and somewhat cigar shaped.
