The galaxy appears to be a disk galaxy, observed at a moderate inclination, though closer to edge-on. There is a central bulge that is relatively prominent and appears to be comprised of older stellar populations based on its yellowish color. Fainter light from the outer disk also seems to be of similar color, indicating aging populations, which could indicate a suppressed star-formation rate. The disk exhibits some irregularities, with subtle disturbances that could potentially be the result of a minor interaction or internal dynamics. There is a slight hint of tidal features or an extended halo, but the image resolution makes it hard to discern any details of these features. Based on the smoothness of the light distribution within the disk there appears to be minimal active star formation.
