The object presents as an elongated, diffuse structure. Its dominant color is blue, indicating a relatively high population of young, hot stars. The luminosity appears to be somewhat unevenly distributed across the galaxy's body. There is evidence of potential disturbances in the galaxy's morphology. Although its form appears primarily smooth in nature, the object's apparent asymmetry and subtly distorted shape may suggest minor tidal interactions or recent merger events. A slight extension or tail-like feature may be present on one side, further hinting at gravitational interactions. This galaxy requires further examination to fully characterize its structural features and evolutionary history.
