The galaxy presents as an elongated, disk-like structure, seen nearly edge-on. A central bulge is evident, appearing more concentrated and yellowish in color, suggesting an older stellar population. The disk component shows a bluer hue, which indicates the presence of younger, hotter stars and ongoing star formation. There is dust obscuration, with dark lanes hinted in the disk, and a smooth radial distribution of light without prominent spiral arms. The overall impression is that of a relatively quiescent galaxy with a moderate level of star formation primarily occurring in the disk region.
