The galaxy appears to be a spiral galaxy, viewed at a relatively high inclination. A central bulge component is prominent and exhibits a yellowish hue, suggesting an older stellar population. Surrounding the bulge, a disk is visible, displaying spiral arm structure. The spiral arms appear somewhat patchy, potentially indicating active star formation regions within the disk. The overall color of the disk is bluer than the bulge, indicating the presence of younger, hotter stars. The galaxy's shape is generally elliptical, but some distortion could be present due to internal dynamics. There are indications of ongoing star formation, but at a moderate rate. The galaxy is not strongly interacting with any other galaxy, appearing relatively isolated. The overall impression is of a mature spiral galaxy with moderate star formation activity and a relatively smooth, undisturbed morphology.