The galaxy appears to be a relatively compact object with an apparent semi-major axis of approximately 3 arcseconds, suggesting a physical size on the order of several kiloparsecs given its redshift. The overall color is bluish, indicating the presence of a young stellar population and ongoing star formation, albeit likely at a moderate rate. The morphology seems intermediate between elliptical and disk-like; while there's a general smoothness to the light distribution, subtle irregularities suggest possible faint spiral arm features or minor disturbances, potentially due to an interaction with another galaxy. The galaxy does not appear perfectly round and has a slightly elongated shape. It could be the result of a recent merger or gravitational interaction that is distorting its shape. Further observations are needed to confirm these possibilities.
