This galaxy presents as a relatively small, disk-shaped object viewed at a moderate inclination. There is a bright, concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the bulge, a flattened disk extends outwards. The disk appears to have some spiral structure although this is not very pronounced in the image. There is possible evidence of reddening at the edges of the disk. Faint, diffuse blue light emanates from the region surrounding the central bulge and is consistent with the presence of younger stars, perhaps in a halo. There is evidence of minor disturbance in the outer disk suggesting an earlier merging event. Overall, the galaxy appears to be undergoing relatively quiescent evolution.
