The galaxy presents as a relatively small, elongated structure with a distinct central bulge. The light distribution suggests a smooth morphology with an observed disk.

There is evidence of possible disturbances or interactions. A faint, somewhat irregular extension or tidal tail-like feature appears to emanate from one side. Hints of possible merging events are suggested by the color and structural asymmetry of the galaxy's central region. Specifically, the nucleus presents a concentration of light, suggesting either a significant star formation event or an active galactic nucleus. A potential merger is also supported by the bending of the galaxy's arm. The overall color suggests the galaxy contains populations of both older and younger stars.