The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. Its morphology seems to be dominated by a spheroidal component. There is a noticeable lack of distinct spiral arm features or a well-defined disk. The galaxy exhibits a yellowish-orange hue, suggesting an older stellar population and lower rate of star formation activity. The shape is generally rounded, with perhaps a slight elongation. No significant signs of recent merging or tidal disturbances are visibly apparent in the image.
