The galaxy presents as a smooth, elongated structure, exhibiting a prolate spheroidal shape. The central region is characterized by a concentrated, bright, yellowish-white core, suggesting a high stellar density and potentially an older stellar population. Moving outward from the core, the color transitions towards a bluer hue. This indicates a more extended distribution of younger, hotter stars in the outer regions. The overall smoothness and lack of distinct features, such as spiral arms or dust lanes, suggest that this galaxy may be an elliptical galaxy. Faint outer regions fade gradually into the background. There are no prominent signs of ongoing merging activity or tidal disturbances.
