The galaxy presents as a luminous, relatively smooth object with a noticeable bulge. It exhibits an elliptical morphology, appearing flattened rather than perfectly spherical. The central region displays a strong concentration of light, indicative of a dense stellar population. There is a suggestion of a disk component, possibly viewed edge-on, contributing to the overall flattened shape. The colors are generally consistent with an older stellar population; yellowish-orange hues are dominant, with hints of bluer light potentially indicating pockets of recent star formation. No significant tidal features or signs of a major ongoing merger are apparent, although there might be some minor irregularity in its shape. The estimated mass indicates a large galaxy, and the inferred star formation rate is relatively low.
