The galaxy presents an elongated, disk-like morphology. It exhibits a smooth, centrally concentrated light distribution with a moderate color gradient. The central region appears more yellow and concentrated, suggesting an older stellar population. Moving outward from the core, the disk becomes fainter and appears slightly bluer in color. No distinct spiral arm structure is visible in this image. There is no strong evidence of a major ongoing merger or significant tidal disturbances based on the galaxy's overall morphology, although minor asymmetries cannot be ruled out without higher resolution imaging. The size of the galaxy appears moderate, consistent with a galaxy of significant stellar mass. Overall, the galaxy appears to be an intermediate to massive system that is in an advanced stage of evolution.