The galaxy presents as a relatively compact object with an overall lenticular morphology. It has a bright, concentrated central bulge, approximately spherical in projection, which appears to smoothly transition into the surrounding disk. The disk structure is subtly visible, appearing somewhat elongated. There are hints of possible disturbances in the outer disk. The system's color profile suggests a relatively mature stellar population. The smooth transition from bulge to disk, combined with the subtle features in the disk, might indicate a recent or ongoing minor merger event. A more thorough analysis would require spectroscopic data to determine redshift, age, and composition.
