The galaxy presents as a system with both smooth and featured components. A central, relatively bright, and smoothly distributed light concentration is evident, likely representing the bulge of the galaxy. This core exhibits a yellowish-orange hue, indicative of an older stellar population. Surrounding the central bulge is a fainter, more extended disk-like structure. The disk shows hints of bluer light, potentially from younger, hotter stars formed in regions of active star formation. Some subtle irregularities or features are visible within the disk, possibly indicating spiral arm segments or disturbances. Overall, the galaxy appears moderately massive with an ongoing low level of star formation activity. The shape is somewhere between round and oval, showing a tendency towards being rounded. There is no obvious sign of an active major merger. However, there is a small probability of either a minor disturbance or a minor merger is underway.
