The galaxy presents an elongated morphology, appearing somewhat flattened and disk-like. The light distribution suggests a central concentration, possibly indicating a bulge component. However, the image resolution limits a precise determination of the bulge-to-disk ratio.

Distinct color gradients are observable. The central region exhibits a greenish hue, possibly indicative of active star formation or ionized gas. Surrounding this area is a more diffuse, yellowish-orange region, potentially signifying an older stellar population.

There are visual indications of possible disturbances in the galaxy's structure. It is not immediately evident whether these are due to tidal interactions, internal dynamics, or imaging artifacts. A more in-depth analysis is needed to understand the features and potential implications. Overall, the galaxy appears to exhibit characteristics of both smooth and irregular morphologies, potentially representing an intermediate stage of galactic evolution.
