The galaxy appears to be a lenticular or early-type spiral galaxy, elongated in shape with a high axial ratio, suggesting it is viewed at a significant inclination. There is a central bulge that is fairly luminous and appears yellowish, indicating a population of older stars. The galaxy's disk is relatively smooth, with minimal evidence of prominent spiral arms or significant dust lanes. The light distribution in the outer regions is diffuse, making it difficult to discern finer details within the disk. The overall color suggests a relatively quiescent galaxy with a low star formation rate and dominant older stellar population. 
