This galaxy appears to be a relatively smooth, elliptical structure with a concentrated central bulge. It exhibits a notable lack of defined spiral arms or significant dust lanes. The light distribution suggests a centrally concentrated luminosity profile, fading gradually towards the outer edges. The overall color is slightly redder, indicating a population of older stars and potentially lower ongoing star formation. There might be some subtle evidence of a faint, extended halo, although it's difficult to discern due to image quality. Based on the roundness, it likely exists on the elliptical to S0 spectrum. There is no obvious merger activity or tidal features.
