The observed galaxy exhibits a disk-like morphology, viewed at a moderate inclination angle. There is a bright, concentrated central bulge that appears to be roughly spherical in shape, possibly indicating an older stellar population within the nuclear region. The disk component displays some complexity in its structure. While primarily smooth, there are subtle indications of some non-uniformity in its brightness profile. The overall color distribution suggests a slightly bluer hue in the outer regions of the disk, with an increased concentration of redder colors toward the center and within the bulge. There is also some evidence of a potential minor interaction or disturbance that could be influencing the galaxy's structure.
