This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. Its overall shape is elongated, being significantly more extended along one axis than the other, though not extremely so. The galaxy exhibits a radial color gradient, with the central region displaying a distinct yellowish-orange hue, suggesting an older stellar population dominated by red giant stars. This coloration gradually fades toward the outer regions, transitioning to a slightly bluer tone, potentially indicating the presence of some younger, bluer stars, or simply less dust obscuration. No spiral arms or significant dust lanes are discernible. There is no evidence of any major ongoing merger activity or significant tidal disturbances. The galaxy appears to be a relatively isolated system.
