The galaxy presents as a somewhat face-on spiral, or perhaps a lenticular galaxy with a significant bulge. The central bulge appears bright and is a yellow-gold color, suggesting an older stellar population. Surrounding the bulge is a fainter disk, showing traces of spiral arm structure. These arms exhibit a bluer hue compared to the bulge, hinting at the presence of younger, hotter stars and ongoing star formation within the disk. The overall morphology indicates the galaxy is relatively undisturbed, lacking strong tidal features or signs of a major merger event. The galaxy is moderately massive, with a relatively low star formation rate for its size, suggesting it may be in a transitional phase of its evolution.
