The galaxy appears as a slightly elongated, face-on spiral or lenticular galaxy. It exhibits a bright, concentrated central bulge that transitions smoothly into a less defined disk. The color profile suggests an older stellar population dominates the bulge, presenting as yellowish-white. The disk shows a bluer hue, indicating some ongoing star formation, though it is not particularly pronounced.  There is a very slight indication of spiral arm structure, although they appear faint and somewhat disrupted. There is no apparent central bar, but the disk structure is irregular and has some disturbances. The disk is relatively smooth, as is the bulge. Overall the galaxy does not appear to be particularly active in terms of star formation.
