The galaxy presents as an elliptical morphology with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggesting an older stellar population. There are no discernible spiral arm structures or dust lanes. The overall shape is elongated, with a minor-to-major axis ratio indicating a relatively high degree of ellipticity. There's little evidence of active star formation. Faint outer regions suggest a gradual decline in stellar density with increasing radius. The galaxy doesn't appear to be undergoing any major merger events or significant tidal disturbances.
