The galaxy presents as a spiral type, exhibiting a disk structure that is not quite edge-on but significantly inclined relative to our line of sight.  There's a central bulge that appears moderately prominent, with a gradual transition from the bulge to the disk. The disk shows evidence of spiral arm structure, although the arms are somewhat loosely wound and possibly flocculent.  Star formation appears to be ongoing, as evidenced by the blue hues throughout much of the disk. The colour gradient suggests younger, hotter stars in the outer regions.  A slight asymmetry may indicate a minor tidal interaction or a past merger event, but the overall structure remains relatively undisturbed. The galaxy seems to be neither a pure elliptical, nor a perfectly symmetrical spiral, but instead displays characteristics of a transitional stage, likely resulting in an intermediate mass. There is no indication of an active galactic nucleus from this image alone.
