This galaxy presents as a relatively compact, yet morphologically complex object. The overall color is a mix of redder and bluer tones, suggesting a composite stellar population.

The central region appears amorphous and diffuse, indicative of a bulge, although its precise shape is difficult to discern. Surrounding this central region, faint, disturbed features appear present, most significantly to the upper-left of the galaxy. These features could be tidal debris resulting from a possible recent minor merger event or interaction, or some internal phenomena.

The color gradients suggest ongoing star formation and dust extinction, though the resolution prevents finer details. The overall impression is of a galaxy undergoing some form of dynamical interaction or exhibiting internal activity beyond quiescent stellar evolution. A deeper analysis with higher resolution images and spectroscopic data would be beneficial to confirm the merger hypothesis.
