The galaxy presents as a moderately inclined spiral, possibly transitioning towards a lenticular morphology. A prominent central bulge dominates the visual appearance. The bulge exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population. The disk component is discernible but less pronounced, showing a flattened structure with relatively faint spiral arms. The disk appears dusty, with some obscuration of background light. Overall, the galaxy appears to be relatively massive, with substantial stellar content. The light distribution indicates that this galaxy is quite centrally concentrated.
