The galaxy presents a primarily elongated morphology, viewed at a significant angle. It appears to possess a central bulge region that is more concentrated and exhibits a warmer color. Extending from the bulge are fainter, less defined disk-like features. The disk demonstrates a bluer hue, suggestive of ongoing star formation activity, compared to the relatively redder bulge. There is a subtle hint of asymmetry within the disk, as if it is slightly disrupted or irregular. Overall, the galaxy's structure is suggestive of an early spiral or lenticular type galaxy with a moderate level of star formation occurring within its disk.