This galaxy appears to be a lenticular or possibly an elliptical galaxy, viewed at an oblique angle. It exhibits a smooth, diffuse light distribution, with a high degree of central concentration. The elongated shape suggests a flattened spheroid, consistent with an E6 or E7 elliptical, or an edge-on S0 galaxy. There is no discernible spiral structure or dust lane visible in this image. A slight color gradient can be observed, with a yellowish core, subtly shifting towards redder hues at the outer edges. This color distribution could indicate an aging stellar population within the galaxy, with younger, bluer stars being less prevalent overall. There is no evidence of any major mergers or tidal disturbances affecting its structure.