The galaxy appears to be an elliptical galaxy, elongated in shape, with a smooth, diffuse structure. The central region exhibits a concentrated, bright core indicative of an older stellar population, showing a yellowish-red hue. Moving outward from the center, there's a noticeable transition to a fainter, more diffuse disk or halo structure. This outer region has a slight bluish tint, suggesting the presence of some younger, hotter stars, but it does not appear to be actively forming stars at a high rate. There are no prominent spiral arms or dust lanes visible, further supporting the classification as an elliptical or lenticular galaxy. There is no apparent interaction with other galaxies, as it does not appear to be significantly distorted.
