The galaxy appears to be a relatively small, moderately bright object. The morphology is difficult to ascertain definitively, but it may be a spiral galaxy seen at a high inclination due to the disk-like shape. There is a hint of possible disturbances in its structure, such as asymmetry or faint tidal features. The galaxy exhibits a moderately bright central bulge or core, suggesting a concentration of older stellar populations. The color of the galaxy appears somewhat reddish, implying a population dominated by older stars. Given the possible disturbances, the galaxy may be undergoing or has recently undergone a minor interaction or merger. Further investigation with higher resolution imaging and spectroscopy would be beneficial to confirm its morphological classification and any signs of interactions.
