The galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge that gradually diffuses into a surrounding disk. The light distribution suggests a relatively evolved stellar population, characterized by a yellow-red hue. There is a suggestion of a slight disk structure, but it does not appear to be highly organized or distinctly spiral. No prominent dust lanes or active star-forming regions are immediately apparent within the resolution of the image. The overall appearance is consistent with a galaxy undergoing relatively little star formation. There is a slight indication of some minor disturbance in the galaxy structure, but overall it is a fairly relaxed galaxy.
