The galaxy appears to be an elliptical galaxy. It is characterized by a smooth, centrally concentrated light distribution, with no apparent spiral arms or dust lanes. It exhibits a generally spheroidal shape, leaning more towards round than elongated, with a consistent falloff in intensity from center to edge. The galaxy's light is dominated by yellowish hues, suggesting an older stellar population. There is no indication of any ongoing major merger activity, with minimal signs of tidal tails or morphological disturbances that would indicate a significant interaction with another galaxy. The light profile suggests that the galaxy is reasonably well-settled, and relatively undisturbed.