The galaxy presents as a smooth, elongated structure with a high degree of central concentration. Its color profile suggests an older stellar population, with a dominant yellow-red hue indicating fewer young, hot stars. The galaxy's shape is distinctly cigar-shaped, meaning it appears significantly longer than it is wide. There is no discernible evidence of spiral arms or a prominent disk. Based on the morphological analysis, this galaxy does not appear to be undergoing any major merger activity or show significant signs of disturbance. Overall, the galaxy appears to be a relatively evolved, quiescent system.
