The galaxy appears as a moderately bright object with a slightly elongated, cigar-shaped morphology. The color profile suggests a relatively evolved stellar population, appearing reddish in composite imaging. There is no distinct evidence of spiral arms or other features indicative of active star formation regions within the observable light, rather there is a smooth, centralized glow. Based on the lack of morphological disturbance, the galaxy appears to be relatively isolated, showing no significant signs of recent or ongoing merger activity. The concentration of light towards the center is suggestive of a dense galactic nucleus. The galaxy presents a regular, relaxed structure, indicating a relatively quiescent evolutionary stage.
